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KONINKLIJKE AKADEMIE 


VAN WETENSCHAPPEN 
-- TE AMSTERDAM -:- 


peOckE DINGS OF THE 
SE CRON OF SCIENCES 


VOLUME XVII 


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JOHANNES MULLER :—: AMSTERDAM 
JUNE 1915 


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KONINKLIJKE AKADEMIE 
VAN WETENSCHAPPEN 
-- TE AMSTERDAM -:- 


ER@ChReOUINGS OF THE 
SECBION OF SCIENCES 


VOLUME XVII 
(5) PART — )) 


JOHANNES MULLER :—: AMSTERDAM 
: DECEMBER 1914: : 


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(Translated from: Verslagen van de Gewone Vergaderingen der Wis- en. 
kundige Afdeeling van 30 Mei 1914 tot 28 November 1914. Dl. XXIL) 


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CONTENTS. 


ABEL’s polynomia (On Hermrre’s and). 192. 
ABSORPTION LINES D, and Ds, (On the structure of the). 720. 
ATR-BLADDER (The physiology of the) of fishes. 1088. 
ALBUMINOUs FLUIDS (The identification of traces of bilirubin in). 807. 
ALKALIES (The coloration of some derivatives of Picrylmethylamide with). 647. 
aLLorropy (The) of cadmium. IT. 54, II. 122. [V. 688. V. 1050. 
— of zine. II. 59. ILL. 641. 
— of copper. II. 60. 
— of antimony. I. 645. 
— of lead. 1. 822. Note. 1055. 
— of potassium. I. 1115. 
— of bismuth. Il. 1236. 
— (The application of the theory of) to electromotive equilibria. IT. 37, IIT. 680. 
— (The metastability of metals in consequence of) and its significance for Chemistry, 
Phyics and Technics. 200. III. 926. LV. 1238. 
— (The metastable continuation of the mixed crystal series of pseudo-components 
in connection of the phenomenon). II. 672. 
ALMOND (Gummosis in the fruit of the) and the Peachalmond as a process of normal 
life. 810. 
amipEs of gz-oxyacids (Action of sodium-hypochlorite on). 1163. 
ammonra (On the interaction of) and methylamine on 2.3.4-trinitrodimethylaniline. 
1034. 
ammonta-water (The system), 182. 
AMORPHOUS CARBON (The decoloration of fuchsin-solutions by). 1322. 
Anatomy. P. Réraic and C. U. Arrins Kappers: “Further contributions to our 
knowledge of the brain of Myxine glutinosa”. 2. 
— ©. Winker: “A case of occlusion of the arteria cerebelli posterior inferior”. 914. 
— J. Borke: “On the termination of the efferent nerves in plain muscle-cells, 
and its bearing on the sympathetic (accessory) innervation of the striated muscle- 
fibre”. 982. 


— J. Borke: “On the mode of attachment of the muscular fibre to its tendonfibres 
in the striated muscles of the vertebrates’. 989. 


— H. A. VERMEULEN: “The vagus area in Camelidae”. 1119. 
ANOMALIES (On SBELIGER’s hypothesis ubout the) in the motion of the inner planets, 23. 
ANTIBODIES (On the formation of) after injection of sensitized antigens. Il. 81S, 
89 
Proceedings Royal Acad, Amsterdam, Vol, XVII, 


ap CONTENTS. 


\NTIGENS (On the formation of antibodies after injection of sensitized). II. 318. 

antimony (The allotropy of). [. 645. 

APOPHYLLITE (On the real symmetry of cordierite and). 480. 

ARIENS KAPPERS (c. U.). v. Kappers (C. U. ARrENs). 

ARSENIC TRISULPHIDE soLs (The connection between the limit value and the concen- 
tration of). 1158. 

ARSENIOUS OXIDE (Compounds of). I. 1111. 

ARTERIA cerebelli posterior inferior (A case of occlusion of the). 914. 

Astronomy. J. Wouter Jr.: “On Seeiiaer’s hypothesis about the anomalies in the 
motion of the inner planets”. 23. 

— W. ve Srrrer: “Remarks on Mr. WotLtyEr’s paper concerning SRELIGER’s 
hypothesis”. 33. 

— W. ve Sitrer: “The figure of the planet Jupiter”. 1047. 

— W. vr Sirrer: “On the mean radius of the earth, the intensity of gravity and 
the moon’s parallax”. 1291. 

— W. ve Srrrer: “On isostasy, the moments of inertia and the compression of 
the earth”. 1295. 

— VW. pe Srrver: ‘The motions of the lunar perigee and node and the figure of 
the moon”. 1309. 

ATEN (A. H. Ww.) and A. Smivs. The application of the theory of allotropy to electro- 
motive equilibria. If. 37. III. 680. 

ATLANTIC OCEAN (On the relation between departures from the normal in the strength 
of the trade-winds of the) and those in the waterlevel and temperature in the 
Northern Kuropean seas. 1147. 

atomic Forces (The caleulation of the molecular dimensions from the supposition of 
the electric nature of the quasi-elastic). 877. 

BAA T (W. c. DB) and F,A, H. Scurernemakers. The system : copper sulphate, copper 
chlorid, potassium sulphate, potassium chlorid and water at 30° C. 533. 

— On the quaternary system KCl—CuCl,—BaClo—H,O. 781. 
— Compounds of the arsenious oxide. I. 1111. 

BACKER (H. J.) and A. P. N. Francurmont. The coloration of some derivatives of 
picrylmethylamide with alkalies. 647. 

— z-Sulpho-propionie acid and its resolution into optically active isomerides. 653. 

BAKHUYZEN (H.G. VAN DE SANDE). Comparison of the Dutch platinum- 
iridium Metre N°. 27 with the international Metre MM as derived from the 
measurements by the Duth Metre Commission in 1879 and 1880, and a prelimi- 
nary determination of the length of the measaring-bar of the French base 
apparatus in international metres. 311. 

~- N. Witpeporr and J. W. Dteeertnk: “Comparison of the measuring bar 
used in the base measurement at Stroe with the Dutch Metre N® 27. 300. 

BASE MEASUREMENT (Comparison of the measuring bar used in the) at Stroe with the 
Dutch Metre No. 27. 300. 

BEEGER (N. G W. H.). On Hermrre’s and ABEL’s polynomia, 192. 

BENZENE DERTVATIVES (The replacement of substituents in). 1027, 


COP ND ky) Nat Ss. Lent 


BENZENES (The nitration of the mixed dihalogen), 846. 


BEIJERINCK (mM. w.). Gummosis in the fruit of the Almond and the Peachalmond 
as a process of normal life. 810. 


BILIRUBIN (The identification of traces of) in albuminous fluids. 807. 


BINARY MIXTURES (Isothermals of monatomic substances and their). XVI. 275. 
— (Isothermals of di-atomic substances and their). XV. 950. XVI. 959. 
BINARY SYSTEM (On unmixing in a) for which the three-phase pressure is greater than 
the sum of the vapour tensions of the two components, 834. 
BismutH (The allotropy of). II. 1236. 
BOEKE (J.). On the termination of the efferent nerves in plain muscle-cells and its 
bearing on the sympathetic (accessory) innervation-of the striated muscle-fibre. 982. 
— On the mode of attachment of the muscular fibre to its tendonfibres in the 
striated muscles of the vertebrates. 939. 
— presents a paper of Dr. A. B. Droocierver Forruyn: “The decoloration of 
fuchsin-solutions by amorphous carbon”. 1322. 
BOER (s. DE). On the heart-rhythm. 1075 IL. 1135. 
BOESEKEN (J.). On catalyse. 546. 
— and W. D. Coney. The reduction of aromatic ketones. II!. Contribution to the 
knowledge of the photochemical phenomena. 849. 
BOILING PoINTs (The influence of the hydration and of the deviations from the ideal 
gas-laws in aqueous solutions of salts on the solidifying and the). 1036, 
BOIs (H. DU). Modern electromagnets, especially for surgical and metalJurgic 
practice. 468. 
— The universality of the Zpeman-effect with respect to the Srark-ellect in canal- 
rays. 873. 
BOKHORST (s. c.) and A. Smits. On the vapour pressure lines in the system phos- 
phorus. Il. 678. III. 962. 
— Further particulars concerning the system phosphorus. 973. 
BOLK (4.) presents a paper of Dr. P. Rorate and Dr. C. U. Ariens Kapprrs: 
“Further contributions to our knowledge of the brain of Myxine glutinosa”. 2. 
— presents a paper of Dr. H. A. Vermeunen: “The vagus area in Camelidae”. 1119, 
BOSCH (J. C, VAN DEN) and Erns? Conen. The allotropy of antimony, I. 645. 
Botany. Miss Lucie C. Dover: “Euergy transformations during the germination of 
wheat-grains’’. 62. 
— M. W. Betertnck: “Gummosis in the fruit of the Almond and the Peachal- 
mond as a process of normal life”. 810, 
— C. E. B. Bremexame: “The mutual iufluence of phototropic and geotropic 
reactions in plants”. 1278. 
BratN of Myxine glutinosa (Further contributions to our knowledge of the). 2. 
uravats (The theoty of) (on errors in space) for polydimensional space with 
applications to correlation (Continuation). 150. 
BREMEKAMP (c. E. B.). On the mutual influence of phototropic and geotropic 
reactions in plants. 1278, 


89* 


IV CONTENTS. 


BROUWER (u. A.). On the granitie area of Rokan (Middle-Sumatra) and on contact 

phenomena in the surrounding schists. 1190. 

BRUTIN (G, DB). A erystallized compound of isoprene with sulphur dioxide. 585. 

— and Ernst Couey. The metastability of the metals in consequence of allotropy, 
and its significance for Chemistry, Physies and Technics. III. 926. 

BiicHNER (x. u.) and L. K. Wotrr. On the behaviour of gels towards liquids and 
the vapours thereof. Il. 92. 

capmtum (The allotropy of). IL, 54. ILL. 122. IV. 638. V. 1050. 

CAMELIDAR (The vagus area in). 1119. 

cANAL-RAYS (The universality of the ZeeMAN-ellect with respect to the Srark-effect 
in). 873. 

CAPILLARY PREssURE (On the measurement of the) in a soap-bubble. 946, 

CAPILLARITY (Measurements on the) of liquid hydrogen. 528. 

caTALYSE (On). 546. 

CHEMICAL constanr (The) and the application of the quantumtheory by the method 
of the natural vibrations to the equation of state of an ideal monatomic gas. 20. 

Chemistry. A. Smivs and A. H. W. Aven: “The application of the theory of allotropy 
to electromotive equilibria”. IL. 37. ILI. 680. 

— E. Coney and W. D. Hetperman: “The allotropy of cadmium, IL. 54, IIT. 122. 
IV. 638. V. 1050. 

— FE. Commn and W. D. Hetprerman: “The allotropy of zine.” IT. 59. IIL. 641. 

— E. Conen and W. D. Herperman: “The allotropy of copper”. II. 60. 

— F. A. H. Scureremakers: “Equilibria in ternary systems’, XV, 70. XV1. 169. 
XVIT. 767. XVIII. 1260. 

— L. k. Worrr and EK. H. Biicuner: “On the behaviour of gels towards liquids, 
and the vapours thereof”. IL. 92. 

— A. Smrrs and 8. Postma: “The system ammonia-water’’. 182. 

— Ernst Conen: “The metastability of the metals in consequence of allotropy and 
its significance for Chemistry, Physics and Technics’. 200. 

— F. M. Janepr and Ant. Sirmex: “Studies in the field of Silicate-chemistry”. 
I}. 239. TIT. 251. 

— I. M. Jarcrr: “The temperature-coefticients of the free surface-energy of liquids 
at temperatures from —80° to 1650° C. I. 329. F. M. Jazerer and M. Surv, 
IT. 365. ILL. 386. F. M. Jananr and J. Kany, IV, 395. F. M. Janorr. V. 405. 
VI. 416. VII. 555. VIII. 571. 

— I. A. H. Scaremyemakers and Miss W. C. pg Baar: “The system: copper 
sulphate, copper chlorid, potassium sulphate, potassium chlorid and water at 
30° C.” 533. 

— J. Borsrxen: “On catalyse”. 546. 

— G. pe Bruin: “A erystallized compound of isoprene with sulphur dioxide”, 585, 

— H. R, Kruyt: “Current potentials of electrolyte solutions”. 615. 

— H. R. Kruyt: “Electric charge and limit value of colloids”. 623. 


— Erxst Coney and J, C van pen Boscu: “The allotropy of antimony”. I, 645, 


CONTENTS. v 


Chemistry. A. P. N. Francurmontr and H. J. Backer: “The coloration of some deri- 
vatives of Picrylmethylamide with alkalies”. 647. 

— A. P.N. Francurmontr and H. J. Backrr: “2 Sulpho-propionic acid and its 
resolution into optically active isomerides”. 653. 

— A. Smits: “The metastable continuation of the mixed crystal series of pseudo- 
components in connection with the phenomenon allotropy”. [L. 672. 

— A. Smrrs and 8. C. Bokuorsr: “On the vapour pressure lines of the system 
phosphorus”. If. 678. 

— F, EH. C. Scugrrer;: “On gas equilibria and a test of Prof. v. p. Waats Jr.s 
formula”, I, 695, Lf. 1011. 

— W. Rernpers: “Equilibria in the system Pb-S-O, the roasting reaction 
process”. 703. 

— F. A. H. Sctretnemakers and Miss W. C. pe Baar: “On the quaternary 
system KCl-CuClo-BaCl2-H.0”. 781 

— Ernst Conen and W, D, Heiperman: “The allotropy of lead’, 822. Note. 1055. 

— A. F. Houtemaw: “The nitration of the mixed dihalogenbenzenes”. $46. 

— J. Borsexen and W. D, Conen: “The reduction of aromatic ketones. III, Contri- 
bution to the knowledge of the photo-chemical phenomena”. 849. 

— Ernst Couen and G. ve Bruin; “The metastability of the metals in conse- 
quence of allotropy and its significance for Chemistry, Physics and Technics”. 
Ill. 926. 

— A Smits and 8S. ©. Bokuorst: “On the vapour pressure lines of the system 
phosphorus”. If. 678. I[f. 962. 

— A. Smits and 8, C, Bokuorst: “Further particulars concerning the system 
phosphorus”. 973. 

— A. F. Hotieman: “The replacement of substituents in benzene derivatives’. 1027. 

— P. van Romburcu and Miss D. W. Wensink: ‘On the interaction of ammonia 
and methylamine on 2.3,4.-trinitrodimethylaniline”. 1034. 

— C. H. Sturrer: “The influence of the hydration and of the deviations from the 
ideal gas-laws in aqueous solutions of salts on the solidifying and the boiling 
points”. 1036. 

— Miss Apa Prins: ‘On critical end-points and the system ethanenaphtalene”’. 1095. 

— F. A. H. Scursinemakers and Miss W. C. pt Baat: “Compounds of the 
arsenious oxyde”. L111. 

— Ernst Conen and 8. Wourr: “The allotropy of potassium”. I. 1115. 

— H. R. Kruyr and Jac. van per Spex: ‘The connection between the limit 
value and the concentration of arsenic trisulphide sols”, 1158. 

— R. A. Weerman: “Action of sodium hypochlorite on amides of z-oxyacids”’. 1163. 

— FE. M. Jarcer: “Researches on Pasteur’s principle of the connection between 
molecular and physical dissymmetry”. I. 1217. 

— Ernst Conen: “The allotropy of bismuth”. [I. 1236. 

— Ernsr Couen and W. D. HELpermMan: “The metastability of the metals in 
consequence of allotropy and its significance for Chemistry, Physics and Tech- 
nics”, IV, 1238. 


VI CONTENTS. 


Chemistry. A. W. k. pp Jone: “Action of sunlight on the cinnamie acids”. 1274. 
CINNAMIC aciDs (Action of sunlight on the). 1274. 
crncLes (Systems of) determined by a pencil of conics. 1107, 
COUEN (ERNST). The metastability of the metals in consequence of allotropy, and 
its significance for Chemistry, Physics and Technics, II. 200. 
— presents a paper of Dr. H. R. Kruyr: “Current potentials of electrolyte 
solutions”. 615. 
— presents a paper of Dr. H. R. Kruyt: “Electric charge and limit value of 
colloids”. 623, 
— presents a paper of Dr. H. R, Kruyr and Jac. vAN per Spek: “The connection 
between the limit value and the concentration of arsenic trisulphide sols”. 1158. 
— The allotropy of bismuth. IL. 1236. 
— and J. C. van pen Boscu. The allotropy of antimony. I. 645. 
— and G. pe Bruin. The metastability of the metals in consequence of allotropy 
and its significance for Chemistry, Physics and Technics. III. 926. 
— and W. D. Hexperman. The allotropy of Cadmium. IL. 54, ILL. 122. LV. 638. 
V. 1050. 
— The allotropy of zine. If. 59. ILI. 641. 
— ‘The allotropy of copper. IL. 60. 
— The allotropy of lead. I. 822. Note 1055. 
— The metastability of the metals in consequence of allotropy and its significance 
for Chemistry, Physics and Technics, IV. 1238. 
— and S. Wotrr. The allotropy of potassium. L. 1115. 
COMUEN (w. D.) and J. Borsnxen. The reduction of aromatic ketones. [II. Contri- 
bution to the knowledge of the photochemical phenomena. 849, 
coLLorps (Electrie charge and limit value of). 623. 
coLORATION (The) of some derivatives of Picrylmethylamide with alkalies. 647. 
coLtoyurs (On IresNeL’s coefficient for light of different). Ist part. 445. 
compound (A crystallized) of isoprene with sulphur dioxide. 585. 
COMPOUNDS of arsenious oxide. I. L111. 
CONCENTRATION (The connection between the limit value and the) of arsenic trisulphide 
sols. 1158. : 
CONGRUENCE (A bilinear) of rational twisted quinties. 1250. 
CONGRUENCES (Some particular bilinear) of twisted cubics. 1256. 
conics (Systems of circles determined by a pencil of). 1107. 
CONTACT=PHENOMENA (On the granitic area of Rokan (Middle Sumatra) and on) in 
the surrounding schists. 1190. 
coprer (The allotropy of). II. 60. 
— (Measurements on the specific heat of lead between 14° and 80° K. and of) 
between 15° and 22° K. 894. 
COPPER SULPHATE, Copper chlorid (The system :), potassium sulphate, potassium chlorid 
and water at 30°. 533. 


CORDIERTTE and Apophyllite (On the real symmetry of). 430, 


Gon Tren Ts. VIl 


CORRELATION (The theory of Bravats (on errors in space) for polydimensional space, 
with applications to) (Continuation). 150. 

CORRESPONDING sTATEs (Contribution to the theory of), 840. 

CRITICAL POINT (Vapour pressures of oxygen and) of oxygen and nitrogen. 950. 

CRITICAL QUANTITIES (A new relation between the) and on the unity of all substances 
in their thermic behaviour. 451. 

— (Some remarks on the values of the) in case of association. 598. 

CROMMELIN (ec. 4.) Isothermals of monatomic substances and their binary mix- 
tures. XVI. 275. 

— Isothermals of di-atomic substances and their binary mixtures. XVI, Vapour 
pressures of nitrogen between the critical point and the boiling point. 959. 
— E. Marutas and H. Kameruineu Oxnes. The rectilinear diameter of nitrogen, 953. 

CRYSTAL sERIFS (The metastable continuation of the mixed) of pseudo-components in 
connection with the phenomenon allotropy. LI. 672. 

crysTaLs (On a new phenomenon accompanying the diffraction of RONTGEN rays in 
birefringent). 1204. 

cue (The different ways of floating of an homogeneous). 224. 

cusres (Some particular bilinear congruences of twisted). 1256. 

curves (Characteristic numbers for nets of algebraic). 935. 

— (Characteristic numbers for a triply infinite system of algebraic plane). 1055, 

DECOLORATION (The) of fuchsin-solutions by amorphous carbon. 1322. 

DEEP reflexes (Exaggeration of). 885. 

pensity (On the manner in which the susceptibility of paramagnetic substances depends 
on the). 110. 

— (Accidental deviations of) and opalescence at the critical point of a single 
substance. 793. 

DIAMETER (The rectilinear) of nitrogen. 953. 

DIEPERINK (J. G.), N. Winpesorr and H. G. vaN DE SanpE Bakuuyzen. Com- 
parison of the measuring bar used in the base measurement at Stroe with the 
Dutch Metre N°. 27. 300. 

DIFFRACTION (On a new phenomenon accompanying the) of Rontgen rays in bire- 
fringent crystals. 1204. 

DIFFUSYON COEFFICIENT (The) of gases and the viscosity of gas-mixtures. 1068. 

DISCONTINUITIES (On apparent thermodynamic) in connection with the value of the 
quantity 2 for infinitely large volume. 605. 

DISSYMMETRY (Researches on PastTEUR’s principle of the connection between molecular 
and physical). I, 1217. 

DORSMAN (c.), H. KameruincH Onnes and G. Hoxsr. Isothermals of di-atomie 
substances and their binary mixtures. XV. Vapour pressures of oxygen and critica! 
point of oxygen and nitrogen, 950. 

DOYER (LUCIE c.). Energy transformations during the germination of wheat-grains. 62. 

DROOGLEEVER FORTUYN (a. B.). v. Fortuyn (A, B. DrooGieever). 

DROSTE (J.). On the field of a single centre in Ernsrein’s theory of gravi- 
tation. 998, 


VIII CONTENTS. 


varru (The mean radius of the), the intensity of gravity and the moon’s parallax. 1291. 
— (On isostasy, the moments of inertia and the compression of the). 1295. 

PHRENFeEST (P.) and H. KameRLINGH OnNes. Simplified deduction of the formula 
from the theory of combinations which PLaNck uses as the basis of his radiation- 
theory. 870. 

— On interference phenomena to be expected when RONTGEN rays pass through a 
di-atomie gas. 1184. 
— On the kinetic interpretation of the osmotic pressure. 1241. 

EWRENPEST (t.)—AvaNaSsJEWA, Contribution to the theory of corresponding 
states. 840. 

EINSTEIN’s theory of gravitation (On the field of a single centre in). 998. 

EINTHOVEN (On the theory of the string-galvanometer of). 784. 

ELASTIC DEFORMATION (On the lowering of the freezing point in consequence 
of an). 732. 

ELECTRIC CHARGE and limit value of colloids, 623, 

ELECTRODES (The effect of magnetisation of the) on the electromotive force. 745. 

ELECTROLYTE SOLUTIONS (Current potentials of) 615. 

ELECTROMAGNETS (Modern), especially for surgical and metallurgic practice. 468. 

ELECTROMETER (A new) specially arranged for radio-active investigations. 659. 

ELECTROMOTIVE FORCE (‘Lhe etlect of magnetisation of the electrodes on the). 745. 

ELIAS (G, J.). On the structure of the absorption lines D,; and Dy. 720. 

— On the lowering of the freezing point in consequence of an elastic deforma- 
tion, 732. 
— The etlect of magnetisation of the electrodes on the electromotive force. 745. 

END-POINTS (On critical) and the system ethane-naphtalene. 1095, 

ENERGY- SURFACE (Lhe temperature-coeflicients of the free) of liquids at temperatures 
from —80° C, to 1650° C. 1. 329. If. 365. IIL. 386. LV. 395. V. 405. VI. 416. 
WUE Gibias MANE. by7pl- 

ENERGY-TRANSFORMATIONS during the germination of wheat-grains. 62. 

ENTROPY CONSTANY (Theoretical determination of the) of gases and liquids. 1167, 

EQUATION OF sTaTE (The chemical constant and the application of the quantum theory 
by the method of the natural vibrations to the) of an ideal monatomic gas. 20. 

EQUILIBRIA (The application of the theory of allotropy to electromotive). Il. 37. III. 680. 

— in the system Pb—SO, the roasting reaction process. 703. 
-- in ternary systems. XV. 70. XVI. 169. XVII. 767. XVIII. 1260. 

ERRATUM. 944. L073. 1202. 

ERRORS IN sPACcE (The theory of Bravats, on) for polydimensional space with appli- 
cations to correlation. (Continuation). 150. 

FTHANE-naphtalene (On critical end-points and the system). 1095. 

EUROPEAN SEAS (On the relation between departures from the normal in the strength 
of the trade-winds in the Atlantic Ocean and those in the waterlevel and tem- 
perature in the Northern), 1147. 

BYKMAN (c,) presents a paper of Dr. L. K, Wourr: “On the formation of antibodies 
after injection of sensitized antigens”. IL, 318, 


CRO MN es ONT 8, IX 


FISHES (The physiology of the air-bladder of). 1088. 

FLOSTING (The different ways of) of an homogeneous cube. 224. 

FLoreEs (On the tin of the island of). 474. 

FOLMER (MISS H.). A new electrometer, specially arranged for radio-active 
investigations. 659. 

FONTAINE SCHLUITER (J. J. DE LA). v. ScHLuiter (J. J. pe LA Fonratne). 

FORTUYN (A. B. DROOGLEEVER). The decoloration of fuchsin-solutions by 
amorphous carbon, 1322. 

FRANCHIMONT (4. P. N.) presents a paper of Dr. R. A. WeerMAN: “Action 
of sodium hypochlorite on amides of g-oxyacids”. 1163. 

— and H. J. Backer. The coloration of some derivatives of Picrylmethylamide with 
alkalies, 647. 

— a-sulpho-propionie acid and its resolution into optically active isomerides. 653. 
FREEZING POINT (On the lowering of the) in connection of an elastic deformation. 732. 
FREQUENCIES (The treatment of) of directed quantities. 586, 

FRESNEL’s coefficient (On) for light of different colours. 445. 

FUCHSIN-SOLUTIONS (The decoloration of) by amorphous carbon. 1322. 

FuNcTIONS of HERMITE (On the). 1st part. 139. 

GALLE (ve. H.). On the relation between departures from the normai in the strength 
of the trade-winds of the Atlantic Ocean and those in the waterlevel and tem- 
perature in the Northern European seas. 1147. 

Gas (The chemical constant and the application of the quantum theory by the method 
of the natural vibrations to the equation of state of an ideal monatomic). 20. 

— (On interference phenomena to be expected when Rontgen rays pass through a 
di-atomic). 1184. 

Gass (The diffusion-coefficient of) and the viscosity of gas-mixtures. 1068. 

— (Tueoretical determination of the entropy constant of) and liquids. 1167. 

Gas EQuiLiBriaA (On) and a test of Prof. v. p. Waaus Jr.’s theorema.]. 695. IL. 1011. 

Gas-Laws (The influence of the hydration and of the deviations from the ideal) in 
aqueous solutions of salts on the solidifying and the boiling points. 1036. 

GaS-MINTURES (The diffusion-coefficient of gases and the viscosity of). 1068. 

GeELs (On the behaviour of) towards liquids and the vapours thereof. IT. 92. 

Geodesy. H. G. van De Sande Baknuyzen, N. WiLpEsorR and J. W. Dreperin«k : 
“Comparison of the measuring bar used in the base-measurement at Stroe, with 
the Dutch Metre N® 27”. 300. 

— H. G. van bE Sanpe Baxkauyzen: “Comparison of the platinum-iridium Metre 
No. 27 with the international Metre M as derived from the measurements by 
the Metre-Commission in 1879 and 1880, and a preliminary determination of 
the length of the measuring-bar of the French base-apparatus in international 
metres”. 311. 

Geology. H. A. Brouwer: “On the granitic area of Rokan (Middle-Sumatra) and on 
contact-phenomena in the surrounding schists’. 1190. 

Geophysics. J. P. van pDER Stok: “The treatment of frequencies of directed quanti- 
ties”. 586, 5 


x CONTENTS. 


Geophysics. P. H. Ganié: “On the relation between departures from the normal in the 
strength of the trade-winds of the Atlantic Ocean and those in the waterlevel 
and temperature in the Northern European seas”. 1147. 


GroTROPIC REACTIONS (On the mutual influence of phototropic and) in plants. 1278. 
GERMINATION (Energy transformations during the) of wheat-grains. 62. 


GRANITIC AREA (On the) of Rokan (Middle-Sumatra) and on contact-phenomena in 


the surrounding schists. 1190. 
GRAVITATION (On the field of a single centre in Ernstetn’s theory of). 998. 
Gravity (The mean radius of the earth, the intensity of) and the moon’s parallax. 1291. 


GuMMosis in the fruit (of the Almond and the Peachalmond as a process of normal 
life. 810. 

I1AGA (H.) presents a paper of Miss H. J. Foumer: “A new electrometer, especi- 
ally arranged for radio-active investigations”. 659. 

— presents a paper of Prof. I. M. Jancer: “On a new phenomenon accompanying 
the diffraction of Réntgenrays in birefringent crystals”. 1204. 

— and F. M, Jarcer. On the real symmetry of cordierite and apophyllite. 430. 

HAMBURGER (H. J.) presents a paper of Dr. E, Laqueur: ‘On the survival of 
isolated mammalian organs with automatic function”. 270, 

— presents a paper of Prof. A. A. Hymans van pDeN Bercu and J. J. pe La 
FontaIne Scutuirer: “The identification of traces of bilirubin in albuminons 
fluids”. 807. 

— Phagocytes and respiratory centre, 1325. 

HEART-RHYTHM (On the). 1075. IT, 1135. 
WELDERMAN (Ww. D.) and Ernsr Conen. The allotropy of cadmium, IL. 54, ILL. 
122. IV, 638. V. 1050. 

— The allotropy of zine. IL. 59. 

— The allotropy of copper. II. 60. 

— The allotropy of lead. 1. 822. Note. 1055. 

— The metastability of the metals in consequence of allotropy and its significance 
for Chemistry, Physics and Technics. LV. 1288. 

neLiuM (Further experiments with liquid), [. 12. 278. K. 283. L. 514. N.520. M. 760, 
HERMITE (On the functions of). 1st part. 139. 
— and ABEL’s polynomia (On). 192. 
oF (K) and H. Kamerurnen ONNEs, Further experiments with liquid helium. N. 520, 
HOLLEMAN (A. F.) presents a paper of Dr. L. K. Wourr and Dr. EK. H, Bicaner: 
“On the behaviour of gels towards liquids and the vapours thereof. IL. 92. 

— presents a paper of Prof. J. BoEsEKEN: “On catalyse”. 546. 

— The nitration of the mixed dihalogen benzenes. 846. 

— presents a paper of Prof. J. Borseken and W. D. Couen: “The reduction of 
aromatic ketones, II. Contribution to the kuowledge of the photochemical 
phenomena”. 849, 

— The replacement of substituents in benzene derivatives. 1027. a 

— presents a paper of Dr. C, H. Suurrer: “The influence of the hydration and 


CUGeN DORN T's; xl 


of the deviations from the ideal gaslaws in aqueous solutions of salis on the 
solidifying and the boiling points’. 1036. 
HOLLEMAN (A. F.) presents a paper of Miss ADA Prins: ,,On critical end-points 
and the system ethane-naphtalene’. 1095, 
noustT (G.) and H. KaMertinen Onnes. The measurement of very low temperatures. 
XXIV. The hydrogen and helium thermometers of constant volume down to the 
freezing point of hydrogen compared with each other and with the platinum- 
resistance thermometer, 501. 
— On the electrical resistance of pure metals. IX. 508. 
— Further experiments with liquid helium. M. 760. 
— H. Kameruncu OnnEs and C. Dorsman. Isothermals of di-atomie substances 
and their binary mixtures. XV. Vapour pressures of oxygen and critical point 
of oxygen and nitrogen. 950, 
HOOGEWERFF (s.) presents a paper of Prof, W. Remnpers: “Equilibria in the system 
Pb-S-O, the roasting reactionprocess. 703. 


HULSHOF (H.). On the thermodynamic potential as a kinetic quantity. Ist part. 85, 


HYDRATION (The influence of the) and of the deviations from the ideal gas-laws in 
aqueous Solutions of salts on the solidifying and the boiling points. 1036, 

HYDROGEN (Measurements of isotherms of) at 20° C. and 13.°5 C. 203. 

— (Measurements on the capillarity of liquid). 528. 

HYDROGEN ISOTHERMS (The) of 20° C. and of 15°.5 C, between 1 and 2200 atms. 217. 

Hydrostatics. D. J. Korrewec: “The different ways of floating of an homogeneous 
cube”. 224. 

HYMANS VAN DEN BERGH (a. a.) and J. J. DE wa Fonraine Scuuurrer. The 
identification of traces of bilirubin in albuminous fluids. 807. 

INERTIA (On isostasy, the moments of) and the compression of the earth, 1295. 
INNERVATION (On the termination of the eiferent nerves in plain muscle-cells and 
its bearing on the sympathetic (accessory) ) of the striated muscle-tibre, 982. 

INTEGRAL EQUATIONS (On some). 286, 
INTEGRAL-FORMULA (On an) of STIELTJEs. 829. 
INTERFERENCE-PHENOMENA (On) to be expected when Roéuntgen-rays pass through a 
di-atomic gas. 1184. 
INVOLUTION (A cubic) of the second class, 105. 
— (A triple) of the third class, 134. 
ISOMERIDES (g-Sulpho-propionic acid and its resolution into optically active). 653. 
1soOPRENE (A crystallized compound of) with sulphur dioxide. 585. 
isostasy (On), the moments of inertia and the compression of the earth, 1295, 
ISOPHERMALS of di-atomic substances and their binary mixtures. XV. Vapour pressures 
of oxygen and critical point of oxygen and nitrogen. 950. XVI. Vapour-pressures 
of nitrogen between the critical point and the boiling point. 959. 
— of monatomic substances and their binary mixtures. XVI. 275. 
IsOTHERMS (The hydrogen) of 20° C. and of 15°95 C. between 1 and 2200 atms. 217. 
— of hydrogen (Measurements of) at 20° C. und 1595 ©, 208, 


XII CRONE DL EN DiS: 


JABGER (er. M.). The temperature-coeflicients of the free surface-energy of liquids at 
temperatures from —80° C. to 1650° C, I. 329. V. 405. VI. 416. VIT. 555. 
VHI. 571. 

— On a new phenomenon accompanying the diffraction of Rontgenrays in birefrin- 
gent crystals. 1204. 
— Researches on Pasreur’s principle of the connection between molecular and 
physical dissymmetry. I. 1217. 
— and H Haga. On the real symmetry of cordierite and apophyllite. 430. 
— and Juz. Kaun. The temperature coefficients of the free surface-energy of 
liquids at temperatures from —80° C. to 1650° C, LV. 395. 
— and Ant. Srmex. Studies in the field of silicate-chemistry, If. 239. IIL. 251. 
— and M. J, Suir. The temperature-coefficients of the free surface energy of liquids 
at temperatures from —80° C. to 1650° C. IT. 365. IIL. 386, 
JONG (A. W. kK. DE). Action of sunlight on the cinnamic acids. 1274. 
Jupiter (The figure of the planet), 1047. 


KAUN (JUL) and F. M. Jatcer, The temperature-coefficients of the free surface- 
energy of liquids at temperatures from —80° C. to 1650° C. LV. 395. 


KAMERLINGH ONNES (H.). vy. Onnes (H. KAaMERLINGH). 


KAPPERS (Cc. U. ARIENS) and P. Roratc. Further contributions to our know- 
ledge of the brain of Myxine glutinosa, 2. 

KAPTEYN (J. Cc.) presents a paper of Prof. M. J. van Uven: “The theory of 
Bravais (on errors in space) for polydimensional space, with applications to 
correlation”. Continuation. 150. 

KAPTEYN (w.). On the functions of Hermite. Lst part. 139. 

— presents a paper of Dr. N, G. W. H. Bescer: “On Hermire’s and ABEL’s 
polynomia”, 192. 

— On some integral equations. 286. 

— presents a paper of Prof. M. J. van Uven: “The theory of the combination 
of observations and the determination of the precision, illustrated by means of 
vectors’, 490. 

KEESOM (w. H.). The chemical constant and the application of the quantum theory 
by the method of the natural vibrations to the equation of state of an ideal 
monatomic gas. 20. 

— On the matter in which the susceptibility of paramagnetic substances depends 
on the density. 110. 

— and H. Kamerttncu Onves. The specific heat at low temperatures. I. Measure- 
ments on the specific heat of lead between 14° and 80° K. and of copper 
between 15° and 22° K, 894. 

KetToNES (The reduction of aromatic). III. Contribution to the knowledge of the photo- 
chemical phenomena. $49. 

KINETIC INTERPRETATION (On the) of the osmotic pressure. 1241. 

KINETIC QUANTITY (On the thermodynamic potential as a). 1st part. 85. 

KLUYVER (J. c.). On an integral formula of STIELTJES. 829. 


CONTENTS XI 


KOHNSTAMM (eH.) and kK, W. Watsrra. Measurements of isotherms of hydrogen 
at 20° C. and 159.5 C. 203. 
KORTEWEG (pb. J.). The different ways of floating of an homogeneous cube. 224, 
KRUYT (H. R.). Current potentials of electrolyte solutions. 615. 
— Electric charge and limit value of colloids. 623. 
— and Jac. van DER Spex. The connection between the limit value and the 
concentration of arsenic trisulphide sols, 1158. 


KUENEN (J. e.). On the measurement of the capillary pressure in a soap-bubble. 946. 
— The diffusion-coefficient of gases and the viscosity of gas-mixtures, 1068. 


KUIPER JR, (K.). Lhe physiology of the air-bladder of fishes. 1088. 


KUYPERS (H. A.) and H. KaweruincH OnNeEs. Measurements on the capillarity of 
liquid hydrogen. 528. 

LAAR (J. J. VAN). A new relation between the critical quantities and on the unity 
of all substances in their thermic behaviour. 451. 

— Some remarks on the values of the critical quantities in case of association. 598. 

— On apparent thermodynamic discontinuities in connection with the value of the 
quantity 4 for infinitely large volume. 606, 

— The calculation of the molecular dimensions from the supposition of the electric 
nature of the quasi-elastic atomic forces. 877. 

LAQUEUR (&). On the survival of isolated mammalian organs with automatic 
function. 270. 

LEAD (The allotropy of). I. 822. Note. 1055. 

— (Measurements on the specific heat of) between 14° and 80° k. and of copper 
between 15° and 22° K, 894. 

LIGHT (On FResNEL’s coefficient for) of different colours. 445. 

LIMIT VALUE (Electric charge and) of colloids. 623. 

— (The connection between the) and the concentration of arsenic trisulphide 
sols. 1158. 

11auIps (On the behaviour of gels towards) and the vapours thereof. II, 92. 

— (Theoretical determination of the entropy constant of gases and). 1167. 

— (The temperature-coefficients of the free energy-surface of) at temperatures from 
—80° C. to 1650° C. I. 329. IL 365. ILL. 389. LV. 395. V. 405. VI. 416. VII. 
556. VILL. 571. 

LORENTZ (H. A.) presents a paper of Dr. J. J. van Laar: “A new relation between 
the critical quantities and on the unity of all substances in their thermic 
behavtour’. 451. 

—- presents a paper of Dr. J. J. van Laan: “Some remarks on the values of the 
critical quantities in case of association’’. 598. 

— presents a paper of Dr. J. J. van Laan: “On apparent thermodynamic discon- 
tinuities in connection with the value of the quantity 4 for infinitely large 
volume”. 606, 

— presents a paper of Dr. G, J. Evras; “On the structure of the absorption lines 
D, and Ds”, 720. 


XIV CONTENTS. 


LORENZ (H. A.) presents a paper of Dr. G. J. Enias: “On the lowering of the 
freezing point in consequence of an elastic deformation”. 732. 

— presents a paper of Dr. G, J. Extras: “The effect of magnetisation of the elec- 
trodes on the electromotive force”. 745. 

— presents a paper of Dr. L. S. Ornstetn: “On the theory of the string galvano - 
meter of Er1ntHOVEN”. 784. 

— presents a paper of Dr. L. S. Ornstein and Dr. F. Zeentke: “Accidental 
deviations of density and opalescence at the critical point of a single sub- 
stance’. 793. 

— presents a paper of Mrs. T. Eurenrest —AranassJewa : “Contribution to the 
theory of corresponding states’. 840. 

— presents a paper of Dr. J. J. van Laan: “The caleulation jof the molecular 
dimensions from the supposition of the electric nature of the quasi-elastic atomic 
forces”. 877. 

— presents a paper of Mr, J. Droste: “On the field of a single centre in 
ErNsTern’s theory of gravitation”. 998. 

— presents of paper of Mr. H. Terrope: ‘Theoretical determination of the entropy 
constant of gases and liquids”. 1167. 

— presents a paper of Prof, P. Kurmnrest: “On interference-phenomena to be 
expected when R6NTGEN rays pass through a di-atomic gas”. 1184. 

— presents a paper of Prof. P. Eurenrest: “On the kinetic interpretation of the 
osmotic pressure”. 1241. 
LUNAR PERIGEE (The motions of the) and node and the figure of the moon. 1309. 
MAGNETISATION (‘The effect of) of the electrodes on the electromotive force. 745. 
MAMMALIAN ORGANS (On the survival of isolated) with automatic function. 270. 
Mathematics. Jan pe Vries: “A cubic involution of the second class”. 105. 

— Jan pve Vrigs: “A triple involution of the third class”. 134. 

— W. Kapreyn: “On the functions of Hermite”. 3th part. 139. 

— M. J. van Uven: “The theory of Bravats (on errors in space) for polydi- 
mensional space with applications to correlation”. (Continuation). 150. 

— M. J. van Uven: “Combination of observations with and without conditions 
and determination of the weights of the unknown quantities, derived from me- 
chanical principles”. 157. 

— N. G. W. H. Beraer: “On Hermrre’s and AsBet’s polymonia”. 192. 

— W. Kapreyrn: “On some integral equations”. 286. 

— M. J. van Uven: “The theory of the combination of observations and the 
determination of the precision, illustrated by means of vectors”. 490. 

— J. ©. Kivyver: “On an integral formula of Srievtses”. 829. 

—- JAN DE Vrizs: “Characteristic numbers for nets of algebraic curves”. 935, 

— Jan pe Vries: “Characteristic numbers for a triple infinite system of algebraic 
plane curves”. 1055. 

— Jan pr Varies: “Systems of circles determined by a pencil of conics”. 1107. 


— W. van per Woupe: “On Norner’s theorem”, 1245. 
— Jan pe Vries: “A bilinear congruence of rational twisted quintics”. 1250, 


CON TEN T §&. >A 


Mathematics. JAN pe Vries: “Some particular bilinear congruences of twisted cubics”. 
1256. 

MATHIAS (£.), H. Kamertincu Onnes and C. A, Crommenin. The rectilinear 
diameter of nitrogen. 953. 

MEASUREMENT (The) of very low temperatures. XXIV. The hydrogen and helium. 
thermometers of constant volume, down to the freezing point of hydrogen compared 
with each other and with the platinum-resistance thermometer. 501. 

MEASUREMENTS On the capillarity of liquid hydrogen, 528. 

— of isotherms of hydrogen at 20° C. and 1595 C. 203. 

— on the specific heat of lead between 14° and 80° k. and of copper between 
15° and 22° K. 894. 

MEASURING Bar (Comparison of the) used in the base measurement at Stroe with the 
Dutch Metre N® 27. 300. 

— (Comparison of the Dutch platinum-iridium Metre N®%, 27 with the international 
Metre M as derived from the measurements by the Dutch Metre-Commission in 
1879 and 1880, and a preliminary determination of the length of the) of the 
French base-apparatus in international metres. 311. 

MECHANICAL PRINCIPLES (Combination of observations with and without conditions and 
determination of the weights of the unknown quantities derived from). 157. 
METALS (The metastability of) in consequence of allotropy, and its significance for 

Chemistry, Physies and Technics. 200. III. 926. 1V. 1238. 

— (On the electrical resistance of pure). IX. 508. 

METASTABILITY (The) of metals in consequence of allotropy and its significance for 
Chemistry, Physics and Technics. 200. III. 926. IV. 1238. 

METHYLAMINE (On the interaction of ammonia and) on 2. 3. 4.-trinitrodimethylaniline. 
1034, 

METRE No. 27 (Comparison of the Dutch platinum-iridium) with the international 
metre M/ as derived from the measurements by the Dutch Metre-Commission in 
1879 and 1880, and a preliminary determination of the length of the measu- 
ring bar of the French baseapparatus in international metres. 311. 

Mineralogy. H. Haca and I’. M, Jararer: “On the real symmetry of cordierite and 
apophyllite”. 430. 

— C. E, A. Wichmann: “On the tin of the island of Flores”, 474. 

MOLECULAR DIMENSIONS (The calculation of the) from the supposition of the electric 
nature of the quasi-elastic atomic forces, 877. 

MOLENGRAAFF (G. 4. F.) presents a paper of Dr. H. A. Brouwer: “On the 
granitic area of Rokan (Middle-Sumatra) and on contact-phenomena in the sur- 
rounding schists”. 1190. 

moon (The motions of the lunar perigee and node and the figure of the). 1309. 

MOON’S PARALLAX (The mean radius of the earth, the intensity of gravity and the), 1291. 


MUSCLE-CELLS (On the termination of the efferent nerves in plain) and its bearing 
- on the sympathetic (accessory) innervation of the striated muscle-fibre. 982. 


MUSCULAR FIBRE (On the mode of attachment of the) to its tendontibres in the 
striated muscles of the vertebrates, 989, 


XVI CONTENTS. 


MYXINE GLUTINOsA (Further contributions to our knowledge of the brain of). 2. 
NERVE-DISTRIBUTION (On the) in the trunk-dermatoma. 632. 
Nerves (On the termination of the efferent) in plain muscle cells and its bearing on 
the sympathetic (accessory) innervation of the striated muscle-fibre. 982. 
Nets (Characteristic numbers for) of algebraic curves. 935, 
NITRATION (The) of the mixed dihalogen benzenes. 846. 
NITROGEN (Vapour pressures of oxygen and critical point of oxygen and). 950. 
— (The rectilinear diameter of). 953. 
-—— (Vapour pressures of) between the critical point and the boiling point. 959. 
NOTHER’s theorem (On). 1245. 
occLusion (A case of) of the arteria cerebelli posterior inferior. 914. 
ONNES (HW. KAMERLINGH). Further experiments with liquid helium. J. 12. 
278. K. 283. L. 514. 

— presents a paper of Dr. W. H, Kegsom: “The chemical constant and the appli- 
cation of the quantum-theory by the method of the natural vibrations to the 
equation of state of an ideal monatomic gas’. 20. 

— presents a paper of Dr, W. H. Kersom: “On the matter in which the suscep- 
tibility of paramagnetic substances depends on the density”. 110, 

— presents a paper of Dr. C. A. Crommezin: “Tsothermals of monatomic sub- 
stances and their binary mixtures”. XVI. 275. 

— presents a paper of Dr. C. A. Cromme in: “Isothermals of di-atomic substances 
and their binary mixtures”, XVI. 959. 

— C. Dorsman and G. Hotsr. Isothermals of di-atomic substances and their binary 
mixtures. XV. Vapour pressures of oxygen and critical point of oxygen and 
nitrogen. 950. 

— and P. Enerenrest. Simplified deduction of the formula from the theory of 
combinations which PLANoK uses as the basis of his radiation theory. 870. 

— and K. Hor. Further experiments with liquid helium, N. 520, 

— and G. Hotst. The measurement of very low temperatures. XXIV. The hydrogen 
and helium thermometers of constant volume down to the freezing point of 
hydrogen compared with each other and with the platinum-resistance thermo- 
meter. 501. 

— On the electrical resistance of pure metals. 1X. 508. 

— Further experiments with liquid helium, M. 760. 

—and W. H. Keresom. The specific heat at low temperatures. I. Measurements 
on the specific heat of lead between 14° and 80° Kk. and of copper between 
15° and 22° K, 894. 

— and H. A. Kuypers. Measurements on the capillarity of liquid hydrogen. 528. 

— BE. Marutas and C. A. Crommenin. The rectilinear diameter of nitrogen. 953. 

OPALESCENCE (Accidental deviations of density and) at the critical point of a single 
substance. 793. 
ORNSTEIN (4. 8.). On the theory of the stringgalvanometer of ErNTHOVEN. 784. 

— and F. Zerntxe. Accidental deviations of density and opalescence at the critical 
point of a single substance. 793. 


CONTENTS Xvit 


OSMOTIC PRESSURE (On the kinetic interpretation of the). 1241. 
OXYGEN (Vapour pressures of) and critical point of oxygen and nitrogen. 950. 


PARAMAGNETIC SUBSTANCES (On the matter in which the susceptibility of) depends on 
the density. 110. 


PASTEUR’s principle (Researches on) of the connection between molecular and 
physical dissymmetry. I. 1217. 


PEACHALMOND (Gummosis in the fruit of the Almond and the) as a process of normal 
life. 810. 

'Petrography. A. Wicumann: “On some rocks of the island of Taliabu (Sula islands). 226. 

PHAGOCYTES and respiratory centre. 1325. 

PHosPHORUs (On the vapour pressure lines of the system). Il. 678. IIL. 962. 

— (Further particulars concerning the system). 973. 

PHOTOCHEMICAL phenomena (Contribution to the knowledge of the). $49. 

PHOTOTROPIC and geotropic reactions (On the mutual inftuence of) in plants, 1278. 

Physics. H. Kamprimcu Onnes: “Further experiments with liquid helium”. J. 12. 
278. K. 283. L. 514, N. 520. M. 760. 

— W. H. Kersom: “The chemical constant and the application of the quantum- 
theory by the method of the natural vibrations to the equation of state of an 
ideal monatomic gas”, 20. 

— H. Huusuor: “On the thermodynamic potential as a kinetic quantity”. 1st part. 85. 

-- W. H. Kexrsom: “On the manner in which the susceptibility of paramagnetic 
substances depends on the clensity”. 110. 

— Pu. Konnstamm and k. W. Watsrra: “Measurement of isotherms of hydrogen 
at 20° C. and 15° C.” 203. 

— K. W. Watstra: “The hydrogen isotherms of 20° C. and of 15°95 C. between 
1 and 2200 atm.” 217. 

— C, A. Cromme.in: “‘Isothermals of monatomic substances and their binary 
mixtures”, XVI, 275. 

= P. Zeeman: ‘'FResNoL’s coefficient for light for different colours”. 1stpart. 445, 

= J. J. van Laar: “A new relation between the critical quantities and on the 
unity of all substances in their thermic behaviour’. 451. 

= H. vu Bois: “Modern electromagnets, especially for surgical and metallurgic 
practice”. 468, 

= H. Kamerninc Onnes and G, Horsr: “On the measurement of very low 
temperatures. XXIV. The hydrogen and helium thermometers of constant volume, 
down to the freezing-point of hydrogen compared with each other and with the 
platinum resistance thermometer’. 501. 

=— H. Kamerninau Onnus and G. Housr: “On the electrical resistance of pure 
metals ete.”. [X. 508. 

— H. Kamernrnen Onnus and H, A. Kuyerrs: ‘Measurements on the capillarity 
of liquid hydrogen”. 528) 

= J. J. van Laan: “Some remarks on the values of the critical quantities in case 


of association’’. 598. 
90) 
Procéedings Royal Acad. Amsterdam. Vol. XVII, 


XVIII CONTENTS. 


Physics. J. J. van Laar: “On apparent thermodynamic discontinuities in connection 
with the value of the quantity 4 for infinitely large volume’’. 606. 
— Miss H. J. Foumpr: “A new electrometer, especially arranged for radio-active 
investigations”. 659. 
— G. J. Brras: “On the structure of the absorptionlines D,; and ),”. 720. 
— G. J. Evras: “The lowering of the freezing point in consequence of an elastic 


deformation”. 732. 
— G. ap Enras: “The effect of magnetisation of the electrodes on the electromotive 
force”. 745. 
— L. 8. Ornstern: “On the theory of the string-galvanometer of ErytHoven’’. 784. 
— L. 8. Ornsrern and F. Zernike: “Accidental deviations of density and opales- 


cense at the critical point of a single substance”. 793. 


— F. E. C. Scnerrer; “On unmixing in a binary system for which the three 
phase pressure is greater than the sum of the vapour tensions of the two compo- 
nents’. 834. 

— Mrs. T. Exrenrest—Aranasssewa: “Contribution to the theory of corresponding 
states”. 840. 

— P. Burenrest and H, KameruincuH Onnes: “Simplified deduction of the 
formula from the theory of combinations which PLANcK uses as the basis of his 
radiationtheory”. 870. 

— H. pu Bors: “The universality of the Zeeman-elfect with respect to the SrarK- 
effect in canal-rays”. 873. 

— J. J. van Laar: “The calculation of the molecular dimensions from the suppo- 
sition of the electric nature of the quasi-elastic atomic forces”, 877. 

— W. H. Kersom and H. Kameruineu Onnes: “The specific heat at low tempe- 
ratures. I. Measurements on the specific heat of lead between 14° and 80° K, 
and of copper between 15° and 22° K.” 894. 

— J. P. Kunnen: “On the measurement of the capillary pressure in a soap-bubble”. 
946. 

— H. Kamertincu Onnes, C. Dorsman and G. Horst: “Isothermals of di-atomic 
substances and their binary mixtures. XV. Vapour pressures of oxygen and critical 
point of oxygen and nitrogen”. 950. 

— E. Mararas, H. Kameruincn Onneis and C, A. CromMEtiIn: “The rectilinear 
diameter of nitrogen”. 953. 

— ©, A. Crommeniy: “Isothermals of di-atomic substances and their binary mixs 
tures. XVI. Vapour pressures of nitrogen between the critical point and the 
boiling point”, 959, 

«- J, Droste: “On the field of a single centre in ErnsTEty’s theory of gravitation”, 
998. 

«- J, P, Kusnex: “The diffusion coefficient of gases and the viscosity of gasa 
mixtures”. 1068, 

s H: Terropk: “Theoretical determination of the entropy constant of gases and 
liquids”. 1167. 


CROPNELS ENG TCS XIX 


Physics. P. Enrenrest: “On interference phenomena to be expected when Réntgen 
rays pass through a di-atomic gas’. 1184. 
_— F. M. Jazcer: “On a new phenomenon accompanying the diffraction of 

R6ntgen rays in birefringent crystals’. 1204. 
— P. Enrenrest: “On the kinetic interpretation of the osmotic pressure”. 1241. 
Physiology. ££. Laaueur: “On the survival of isolated mammalian organs with auto- 
matic function”. 270. 
—L. K. Wotrr: “On the formation of antibodies after injection of sentizised 
antigens”. II. 318. 
— G. van Risnperk: “On the nerve-distribution in the trunk-dermatoma’’. 632. 
— A. A. Hymans vAN DEN Bereu and J. J. pe ta Fontatne Scauurrur: “The 
identification of traces of bilirubin in albuminous fluids”. 807. 

— I. K. A. Werraetm Satomonson: “Exaggeration of deep reflexes”. 885. 

— S. pe Borer: “On the heart-rhythm”. 1075. If. 1135. 

— A. B. Droocierver Fortuyn: “The decoloration of fuchsin-solutions by amor- 

phous carbon”, 1322. 
— H. J. Hameurcer: “Phagocytes and respiratory centre”. 1525. 
PICRYLMETHYLAMIDE (The coloration of some derivatives of) with alkalies. 647. 
PLANCK (Simplified deduction of the formula from the theory of combinations which) 
uses as the basis for his radiation theory. 870. 

PLANET Jupiter (The figure of the). 1047. 

PLANETS (On SEELIGER’s hypothesis about the anomalies in the motion of the 
inner). 23. 

PLANTs (On the mutual influence of the phototropic and geotropic reactions in). 1278 

poLyNoMIA (On Hermitre’s and ABEL’s). 192. 

PostTMA (s.) and A. Smits. The system Ammonia-water. 182. 

porass1uM (The allotropy of). I. 1115. 

POTASSIUM SULPHATE, potassium chlorid (The system: copper sulphate, copper chlorid) 
and water at 30°. 532. 

POTENTIAL (On the thermodynamic) as a kinetic quantity. Ist part, 85. 

POTENTIALS (Current) of electrolyte solutions. 615. 

PRECISION (The theory of the combination of observations and the determination of 
the), illustrated by means of vectors. 490. 

PRINS (Miss ADA). On critical end-points and the system ethane-naphtalene. 1095. 

PSEUDO-COMPONENTS (The metastable continuation of the mixed crystal series of) in 
connection with the phenomenon allotropy. I. 672. 

quantity 4 (On apparent thermodynamic discontinuities in connection with the value 
of the) for infinitely large volume. 606. 

QuaNnTUM-rtHEORY (The chemical constant and the application of the) by the method 
of the natural vibrations to the equation of state of an ideal monatomic gas). 20 

QUATERNARY sysTEM KCl—CuClz2—BaCl,—H20 (On the). 781. 

auinrics (A bilinear congruence of rational twisted). 1250. 

RADIATION THEORY (Simplified deduction of the formula from the theory of combina- 
tions which PLancK uses as the basis for his). 870. 


XX CONTENTS 


RADIO-ACTIVE investigations (A new electrometer, specially arranged for). 659. 
REPLEXES (Exaggeration of deep). 885. 
REINDERS (w.). Equilibria in the system Pb-S-O, the roasting reaction process. 703. 
RESISTANCE (On the electrical) of pure metals. 1X. 508. 
RESPIRATORY CENTRE (Phagocytes and), 1325. 
ROASTING REACTION PROCESS (f{quilibria in the system Pb-S-O, the). 703. 
rocks (On some) of the island of Taliabu (Sula islands). 226. 
ROKAN (Middle-Sumatra) (On the granitic area of) and on contact phenomena in the 
surrounding schists, 1190. 
ROMBURGH (e. VAN) presents a paper of Prof. F. M. Jareer and Dr. Ant. SimEk: 
“Studies in the field of silicate-chemistry”. Il. 239. ILI. 251. 
— presents a paper of Prof. F. M. Jarcer: “The temperature-coefticients of the 
free surface-energy of liquids at temperatures from —S8U° to 1650° C.” I. 329. 
II. 365. ILI. 886. IV. 395. V. 405. VI. 416. VII. 555. VILL. 571. 
— presents a paper of Mr. G. pr Bruin: “A crystallized component of isoprene 
with sulphur dioxide”. 585. 
— presents a paper of Prof. F, M. Jazcrr: “Researches on Pasteur’s principle of 
the connection between molecular and physical dissymmetry”. I. 1217. 
— presents a paper of Dr. A. W. K. pg Jona: ‘Action of sunlight on the cin- 
namic acids’. 1274. 
— and Miss D, W. Weysinx. On the interaction of ammonia and methylamine 
on 2.3.4,-trinitrodimethylaniline. 1034. 
RONTGEN Rays (On interference phenomena to be expected when) pass through a 
di-atomic gas. 1184. 
— (On a new phenomenon accompanying the diffraction of) in birefringent 
crystals. 1204. 
ROTHIG (p.) and C. U. ArtENs Kappers. Further contributions to our knowledge 
of the brain of Myxine glutinosa. 2. 
RIJNBERK (G. VAN) On the nerve-distribution of the trunk-dermatoma. 6382. 
SALOMONSON (J. K. A. WERVHEIM). Hxaggeration of deep reflexes. 885. 
— presents a paper of Dr. S. p—E Boer: ‘On the heart-rhythm’. 1075. LI. 1135. 
saLts (The influence of the hydration and of the deviations from the ideal gas-laws 
in aqueous solutions of) on the solidifying and the boiling point. 1036. 
SANDE BAKHUYZEN (H. G VAN DE). vy. Bakauyzen (H. G. vaAN DE Sanpg), 
SCHEFFER (Ff. E. c.). On gas equilibria and a test of Prof. v. p. Waats-JR.’s 
theorema. I. 695. Il. 1011. 
— On unmixing in a binary system for which the three-phase pressure is greater 
than the sum of the vapour tensions of the two components. 834, 
SCHLUITER (J. J. DE LA FONTAINE) and A. A. HyMans VAN DEN BERGH. 
The identification of traces of bilirubin in albuminous fluids. 807. 
SCHREINEMAKERS (fF. A. H.). Equilibria in ternary systems. XV. 70. XVI. 
169. XVII. 767. XVIII. 1260. 
— and Miss W. C. pe Baat. The system: copper sulphate, copper chlorid, potas- 
sium sulphate, potassium chlorid and water at 30° C. 533, 


CONTENTS. XXI 


SCHREINEMAKERS (Ff. A. H.) and Miss W. C. pe Baar. On the quaternary 
system KCl-CuClg-BaClo-H,C. 781. 
— Compounds of the arsenious oxide, I. 1111. 
8EEL1GER’s hypothesis (On) about the anomalies in the motion of the inner planets. 23. 
— (Remarks on Mr. WoLtsEr’s paper concerning). 33. 
SILICATE-CHEMISTRY (Studies in the field of). If. 239. III. 251. 

SIMEK (anv) and F, M. Jazcpr. Studies in the field of silicate-chemistry. IT. 
239, IIL. 251. 
SITTER (Ww. DE) presents a paper of Mr. J. Wouter oro: “On SEELIGER’s hypo- 

thesis about the anomalies in the motion of the inner planets”. 23. 
— Remarks on Mr. Woutyer’s paper concerning SrenicEr’s hypothesis. 33. 
— The figure of the planet Jupiter. 1047. 
— On the mean radius of the earth, the intensity of gravity and the moon’s parallax. 1291. 
— On isostasy, the moment of inertia and the compression of the earth. 1295. 
— The motions of the lunar perigee and node and the figure of the moon. 1309 
sLUITER (c. H.). The influence of the hydration and of the deviations from the idenl 
gas-laws in aqueous solutions of salts on the solidifying and the boiling-point. 1036. 
smivt (m.) and F, M. Jancrer. The temperature-coefficients of the free-surface-energy 
of liquids at temperatures from —S0° C. to 1650° C. Il. 365. IIT, 381. i. 
sMits (a). The metastable continuation of the mixed crystal series of pseudo- 
components in connection with the phenomenon allotropy. II, 672. 
— and Aten (A. H. W.). The applicaticn cf tle theory of al’otropy to electro- 
motive equilibria. 11. 37. ILI. 680. 
— and 8S. C. Boxknorst. On the vapour pressure lines in the system phosphorus. {1 
678. III, 962. 
— Further particulars concerning the system phosphorus, 973. 
— and 8, Postma. The system ammoniawater. 182. 
SOAP-BUBBLE (On the measurement of the capillary pressure in a). 946, 
SODIUM-HYPOCHLORITE (Action of) on amides of z-oxyacids. 1163. 
SPECIFIC HEAT (The) at low temperatures. [. Measurements on the specific heat of lead 
between 14° and 80° K. and of copper between 15° and 22° k, 894. 
SPEK (sac. VAN DER) and H. R. Kruyt. The connection between the limit 
value and the concentration of arsenic trisulphide sols. 1158, 
stakK-effect (The universality of the Zeeman-eflect with respect to the) in canal-rays. 873 
sT1ELTJES (On an integral-formula of). 829. 
STOK (J. P. VAN DER). The treatment of frequencies of directed quantities. 586. 
— presents a paper of Mr. P. H. Ga11é: “On the relation between departures 
from the normal in the strength of the trade-winds in the Atlantic Ocean and 
those in the waterlevel and temperature in the Northern European seas.’ 1147. 
STRING-GALVANOMETER (On the the theory of the) of EintnHoven. 784. 
stRoE (Comparison of the measuring bar used in the base measurement at) with the 
Dutch Metre n° 27. 300. 
suBsTANCES (Isothermals of monatomic) and their binary mixtures. XVI. 


275. 
— (Isothermals of di-atomic) and their binary mixtures, XV. 950, XVI, 959. 


NXIT CONTENTS. 


substances (A new relation between the critical quantities and on the unity of all) 
in their thermic behaviour. 451. 

suBsTItuENTS (The replacement of) in benzene derivatives. 1027. 

4-SULPILO-PROPIONIC acrb and its resolution into optically active isomerides. 653. 

SULPHUR DIOXIDE (A erystallized compound of isoprene with). 585. 

SUNLIGHT (Action of) on the cinnamie acids. 1274. 

system PJ-S-O (Equilibria in the), the roasting reaction process. 703. 

— (The) copper sulphate, copper chlorid, potassium sulphate, potassium chlorid and 
water at 30° C. 533. 

— (Characteristic numbers for a triply infinite) of algebraic plane curves. 1055. 

— ammonia—water (The). 182. 

— ethane—naphthalene (On critical endpoints and the). 1095. 

— phosphorus (On the vapour pressure lines in the). IH. 678. [[L 962. 

— phosphorus (Further particulars concerning the). 973. 

vALIABU (Sula islands) (On some rocks of the island of). 226. 

TEMPERATURE (On the relation between departures from the normal in the strength 
of the trade-winds of the Atlantic Ocean and those in the waterlevel and) in 
the Northern European seas. 1147. 

TEMPERATURE-COEFFICIENTS (The) of the free energy surface of liquids at tempera- 
tures from —80° C. to 1650° C. I. 329. IL. 365. ILL 386. LV. 395. V. 405. 
VI. 416. VIL. 555. VIII. 571: 

TEMPERATURES (The measurement of very low). XXLV. The hydrogen and helium 
thermometers of constant volume down to the freezing point of hydrogen com. 
pared with each other and with the platinum-resistance thermometer. 501. 

— (The specific heat at low). [. Measurements on the specific heat of lead between 
14° and 80° K. and of copper between 15° and 22° K. 894. 

TENDONFIBRES (On the mode of attachment of the muscular fibre to its) in the striated 
muscles of the vertebrates. 989. 

TERNARY sYSteMS ([quilibria in). XV. 70. XVL. 169. XVIL. 767. XVIII. 1260. 

TETRODE (u.). Theoretical determination of the entropy constant of gases and liquids. 1167. 

TuEORY of allotropy (The application of the) to electromotive equilibria. I. 37. UL 680. 

— of Bravats (The) (on errors in space) for polydimensional space with applica- 
tions to correlation. (Continuation). 150. 

— (The) of the combination of observations and the determination of the precision, 
illustrated by means of vectors. 490. i 

— of combinations (Simplified deduction of the formula from the) which Pranck 
uses as the basis of his radiation theory. 870. 

— of corresponding states (Contribution to the). 840. 

— of gravitation (On the field of a single centre in Etnsrety’s). 993. 

THERMOMETERS (The hydrogen and helium) of constant volume, down to the freezing 
point of hydrogen compared with each other, and with the platinum-resistan ce 
thermometer, 501. 

TUREE-PHASE PRESSURE (On unmixing in a binary system for which the) is greater 


than the sum of the vapour tensions of the two components. 834. 


CONTENTS. XXIII 


Tin (On the) of the island of Flores. 474. 

TRADE-WINDs (On the relation between departures from the normal in the strength 
of the) in the Atlantic Ocean and those in the waterlevel and temperature in 
the Northern European seas. 1147. 

TRINITRODIMETHYLANILINE (On the interaction of ammonia and methylamine on 
2.3.4.-). 1034. 

TRUNK-DERMATOMA (On the nerve-distribution in the). 632. 

UNMIXING (On) in a binary system for which the three-phase pressure is greater than 
the sum of the vapour tensions of the two components. 83+. 

UVEN (M. J. VAN). The theory of Bravats (on errors in space) for polydimensional 
space with applications to correlation. (Continuation). 150. 

— Combination of observations with and without conditions and determination of 
the weights of the unknown quantities, derived from mechanical principles. 157. 

— The theory of the combination of observations ani the determination of the 
precision, illustrated by means of vectors. 490. 

VAGUS AREA (The) in Camelidae. 1119. 
VAPOUR PRESSURE LtNeés (On thie) in the system puosphorus. IL. 678. ILL. 962. 
VAPOUR PRESSURES of oxygen and critical point of oxygen and nitrogen. 950. 

— of nitrogen between the critical point and the boiling point. 959. 

VAPOUR TENSIONS (On unmixing in a binary system for which the three-phase pressure 
is greater than the sum of the) of the two components. 834. 

vectors (The theory of the combination of observations and the determination of the 
precision, illustrated by means of). 490. 

VERMEULEN (H. A.). The vagus area in Camelidae. 1119. 

VerTEBRATES (On the mode of attachment of the muscular fibre to its tendontibres 
in the striated muscles of the). 989. 

viscosity of gas-mixtures (The diffusion-coefticient of gases and the). 1068. 

VRIES (JAN DE). A cubic involution of the second class. 105. 

— A triple involution of the third class. 13+. 

— presents a paper of Prof. M. J. van Uven: “Combination of observations with 
and without conditions and determination of the weights of the unknown quantities, 
derived from mechanical principles’. 157. 

— Characteristic numbers for nets of algebraic curves. 935. 

— Characteristic numbers for a triple infinite system of algebraic plane curves. 1055. 

— Systems of circles determined hy a pencil of conics, 1107. 

— presents a paper of Dr. W. van per Wouve: “On Noraer’s theorem”. 1245. 

— A bilinear congruence of rational twisted quinties. 1250. 

— Some particular bilinear congruences of twisted cubics. 1256. 

WAALS (J. D. VAN DER) presents a paper of Prof. A. Smits and Dr. A. H. W, 
ATEN: “The application of the theory of allotropy to electromotive equilibria” 
I]. 37. ILI. 680, 
— presents a paper of Dr. H. Hunsuor: “On the thermodynamic potential as a 
kinetic quantity”, Ist. part. 85. 


— presents a paper of Prof. A. Smits and S. Posraa: ‘The system ammonia-water.”” 182, 


XALV CONTENTS. 


WAALS (J. D. VAN DER) presents a paper of Prof. Pu. Kounstamm and kK. W. 
Waustra: “Measurements of isotherms of hydrogen at 20° C. and 1525 C.” 203. 

— presents a paper of Mr. K. W. Waustra: “The hydrogen isotherms of 20° C. 
and of 15°.5 C. between 1 and 2200 atm.”, 217. 

— presents a paper of Prof. A. Smits: “The metastable continuation of the 
mixed erystal series of pseudo-components in connection with the phenomenon 
allotropy”. II. 672. 

— presents a paper of Prof. A. Sirs and S. C. Bokuorst: “The vapour pressure 
lines of the system phosphorus”. II. 678. IIT. 962. 

— presents a paper of Dr. F. E. ©. Scuerrer: ‘On gas equilibria and a test of 
Prof. vaN per Waats Jr.’s formula”. I. 695. IL. 1011. 

—— presents a paper of Dr. FB. E. C. Scnrrrer: “On unmixing in a binary system 
for which the three-phase pressure is greater than the sum of the vapour tensions 
of the components”. 834. 

— presents a paper of Prof. A. Smrvs and 8. ©. Boknorstr: “Further particulars 

concerning the system phosphorus”. 973. 

WAALS JR's theorema (On gas equilibria and a test of Prof.). L695. If, 1011. 

WALs@tRA (xk. w.). The hydrogen isotherms of 20° C. and of 15°5 C. between 1 

and 2200 atm. 217. 

— and Pu. Kounstamm. Measurements of isotherms of hydrogen at 20° C, and 
159.5 C, 2038. 

water (The system ammonia—), 182. 

— (The system: copper sulphate, copper chlorid, potassium sulphate, potassium 
chlorid and) at 30°, 533. 

WATERLEVEL (On the relation between departures from the normal in the strength of 
the trade-winds in the Atlantic ocean and those in the) and temperature in the 
Northern European seas. 1147. 

WEBER (MAX) presents a paper of Dr. K. Kuiper Jr.: “The physiology of the 
air-bladder of fishes’. 1088. 

WEERMAN (k. A.). Action of sodium hypochlorite on amides of ¢-oxyacids. 1163, 
weicuts (Combination of observations with and without conditions and determination 
of the) of the unknown quantities, derived from mechanical principles. 157. 
WENsINK (Miss pv. w.) and P. van RomBurcu. On the interaction of ammonia 

and methylamine on 2.3.4,-trinitrodimethylaniline. 1034. 


WENT (F. A. FP. C.) presents a paper of Miss Lucin C. Dover: “Energy transfor- 
mations during the germination of wheat-grains”. 62. 


— presents a paper of Dr, C. E. B. Bremexame: “On the mutual influence of 
phototropic and geotropic reactions in plants”. 1278. 


WERTHEIM SALOMONSON (I. K. A.) v. Sanomonson (I. K. A. WERTHEIM). 
WHBEAT-GRAINS (Energy transformations during the germination of). 62. 
WICHMANN (a.). On some rocks of the island of Taliabu (Sula islands). 226. 

— On the tin of the island of Flores. 474. 


WILDEBOER (N.), J. G. Drepertnx and H. G. vAN DE SanpE BaknuyzEN. Com- 
parison of the measuring bar used in the base measurement at Stroe with the 
Dutch Metre No. 27. 300. 


CONTENTS. XXV 


WINKLER (c.) presents a paper of Prof. G. van RignBerk : “On the nerve-distri- 
bution of the trunkdermatoma.” 632. 
— A ease of occlusion of the arteria cerebelli posterior inferior. 914. 
WoLFF (L, K.). On the formation of antibodies after injection of sensitized antigens. 
II. 318. 
— and E, H. Bicnner. On the behaviour of gels towards liquids and the vapours 
thereof. II. 92. 
WOLFF (s.) and Ernst Conen. The allotropy of potassium. I. 1115. 
WOLTJER JR. (J.). On Srevicer’s hypothesis about the anomalies in the motion 
of the inner planets. 23. 
WOUDE (Ww. VAN DER). On Noruer’s theorem. 1245. 
ZEEMAN (P.). On FRESNEL’s coefficient for light of different colours, 445. 
ZEEMAN-effect (The universality of the) with respect to the Srark-ellect in canal- 
rays. 873. 
ZERNIKE (f.) and L, S. Ornstein. Accidental deviations of density and opalescence 
at the critical point of a single substance. 793. 
zinc (The allotropy of). Il, 59. III. 641. 
Zoology. K. Kuiper Jr.; “The physiology of the air-bladder of fishes.” 1088. 


de | ie 9 


KONINKLIKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 
of Saturday May 30, 1914. 
Von XVII. 


IS 


President: Prof. H. A. Lorentz. 
Secretary: Prof. P. Zueman. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 30 Mei 1914, DI. XXII1). 


OOyaNy PROD INES 


P. Rérmie and C. U. Armys Karrrrs: “Further contributions to our knowledge of the 
brain of Myxine glutinosa’”. (Communieaied by Prof. L. Bork), p. 2. (With 2 pl.). 

H. Kamervincu Onnes: “Further experiments with liquid helium, J. The imitation of an 
AMPERE molecular current or of a permanent magnet by means of a supra-conductor”, p. 12. 

W. H. Kersom: “The chemical constant and the application of the quantum-theory by the 
method of the natural vibrations to the equation of state of an ideal monatomic gas’, 
(Communicated by Prof. H. Kamerrinon Onnes), p. 20. 

J. Wortses Jr.: “On Srericer’s hypothesis about the anomalies in the motion of the inner 
planets’. (Communicated by Prof. W. DE Sirrer), p, 23. 

W. be Sirrer: “Remarks on Mr. Wortser’s paper concerning SEELIGER’s hypothesis’, p. 33. 

A. Smits and A. H. W. Aten: “The application of the theory of allotropy to electromotive 
equilibria”. If. (Communicated by Prof. J. D. van per WaAats), p. 37. 

Ernst Conrn and W. D. Herperman: “The allotropy of Cadmium”. IT, p. 54. 

Ernst Conen and W. D. Herprerman: “The allotropy of Zine”. II, p. 59. 

Ernst Conen und W. D. Heriperman: “The allotropy of Copper. II, p. 60. 

Lucir C. Dover: “Energy transformations during the germination of wheat grains”. (Com- 
municated by Prof. F. A. F. C. Wenn), p. 62. 

F. A. H. Scuremvemakers: “Equilibria in ternary systems.” XV, p. 70. 

H. Hursnor: “On the thermodynamic potential as a kinetic quantity”. (First part). (Commu- 
nicated by Prof. J. D. van DER WAALS), p. 85. 

L. K. Worr and E. H. Biicuner: “On the behaviour of gels towards liquids and the vapours 
thereof”. (Communicated by Prof. A. F. Horiieman), p. 92. 

Jan DE Vries: “The quadruple involution of the cotangential points of a eubie pencil”, p. 102. 

Jan dE Vries: “A cubic involution of the second class”, p. 105. 

W. H. Kersom: “On the manner in which the susceptibility of paramagnetic substances 
depends on the density.” (Communicated by Prof. H. Kamertincu Onnes), p. 110 

Ernst Conen and W. D, Herperman: “The allotropy of Cadmium IIL’, p. 122. 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


») 
Anatomy. — ‘Further contributions to our knowledge of the brain 
of Myaine gluitinosa.” By P. Rorsic (Berlin) and C. U. Artins 
Kapprrs (Amsterdam). (Communicated by Prof. L. Bork). 


(Communicated in the meeting of March 28, 1914). 


The former of us has given a description of the motor roots and 
nucler in’ Myxine glutinosa and in some Amphibia in Vol. XVI of 
these Proceedings (p. 296). 

For Myxine the topography of the V—VIL nucleus and the spino- 
occipital column has been discussed, and mention was made of the 
absence of the eyemuscle-nuclei and the motor glossopharyngeus. 

For the discussion of the vagus roots reference was made to 
further researches not yet completed at that time, which we should 
accomplish in conjunction. 

It is known that the vagus of Myxine glutinosa has caused 
many difficulties, and before givine our own results we wish 
to review the opinions of former authors, because such a review 
clearly shows the points which give rise to different interpretations. 

It is obvious that in doing so we shall be obliged to deal again 
with other roots of the cranial nerves in Myxine. 

The first deseription of the central nervous system of Myxine 
elutinosa was given by Anpurs Rerzivs ?), who mentions three 
nerves of the Oblongata, the Vagus, a nerve of the labyrinth (Table 
VI le. Fig. 7), a cutaneous branch of this labyrinth nerve (Table 
VI, Fig. 8) and several branches of the V (p. 397, 400 and 401.) 

After A. Rerzivs, Jonannns MUier’*) gave an elaborate description 
of the origin and periferal course of the cranial nerves in Petromyzon, 
Bdellostoma and Myxine. For Myxine he gave a description of the 
Trigeminus, Facialis, Acusticus and Vagus (comp. Fig. 4, 4 and 6 
on Table III |. ¢. 1888). 

It is interesting that he mentions a cutaneous branch of the VII 
(p. 195 Le. 1838), which still wants affirmation, specially since 
Miss Worrnineton *) could not find any but visceral sensory and 
Deere Rerztus, Beitrag zur Anatomie des Ader- und Nervensystems der Myxine 
Glutinosa (Lin.) (Aus d. Abhandlg. d. KGénigl. Sehwedischen Akademie der Wissen 
schaften Jahrgang 1822 H. 2) Meikel’s Archiv fiir Anatomie u. Physiologie 1826 
S. 386—404. 

2) J. Miitter, Ueb. d. eigentiimlichen Bau des Gehdérorgans bei den Cyclostomen, 
mit Bemerkungen itiber die ungleiche Ausbildung der Sinnesorgane bei den 
Myxinoiden Abhandlg. d. Kgl. Akad. d. Wissensch. Berlin 1837 (25. LV. 1836), 
und: Vergleichende Neurologie d. Myxinoiden, ibidem, 1888 (15. IL. 1838). 

3) J. WortHiInaTon: Descriplve Anatomy of tbe Brain and cranial nerves of 
Buellostoma dombeyi (p. 169) Quart. Journ. Miser. Science Vol. 49, 1906. 


3 


motor fibres in the facial nerve of the American Myxinoid Bdello- 
stoma dombeyi. 

After Jou. Minter, Gusrar Rerzius') gave very valuable contri- 
butions which appeared abundantly illustrated in 1881 and 1893. 
It is just the excellent descriptions given by G. Rerzits that show 
how difficult the interpretation of this brain is, for G. Rerzius himself 
emphasizes at the end of his elaborate description of 1893 (p. 63) 
that — though he had been gathering the data concerning the 
brain of this animal for several years, he had not yet succeeded in 
obtaining a complete idea of its exact relations. 

G. Rerzius mentions, as did P. Rérmie in his contribution (1. ¢.), 
the absence of the trochlearis, oculomotorius and abducens. The 
most frontal nerve roots, according to him, are two trigeminal 
branches (p. 60 and Table 24, Fig. 1—3) each provided with a 
spindleshaped ganglion. 

Following on this he finds a small nerve without ganglion (a 
motor nerve consequently) which he considers to be — like Jon. 
Miitiwr — the facial nerve. Close to this nerve he finds a third 
ganglionated root, which he supposes to be a third trigeminus root 
and behind these the two roots of the oetavus occur whieh he had 
already described before (1881): the Ramus anterior and ramus 
posterior acustici. Mueh more backward the vagus roots appear 
without ganglion. Dorsally from these le, however, finds a small 
sensory root with an oval ganglion, which he considers to be a 
sensory vagus root (p. 99). 

After G. Rerzius Sanpers*) took up this subject. Since this work 
was not available for us, we can only quote from it what Hon 
has cited (Il. ¢. infra). 

According to this author Sanpprs found the V, VI, VIII and X 
nerves, but differs in so far from G. Rerztus that he considers some 
roots entering the brain behind the vagus of Rurzius still as vagus 
roots, whilst the latter mentions them as spino-occipital nerves. 

It is Sanprrs’ merit to have first given a detailed«deseription of 
the oblongata-nuclei, which he divides into two cellgroups of which 
one has an entirely central position near the dorsal raphe: “ganglia 
centralia’, and another near the perifery of the bulb: “ganglia latero- 


1) G. Rerzius. Das Gehérorgan d. Wirheltiere Bd. I, Stockholm, 1881; Ueb. d. 
Hypophyse von Myxine Biolog. Untersuchg. Bd. Vi; Das Riickenmark yon Myxine 
Biolog. Untersuchg. N. F. Bd. W. 1891; Das Gehirn und das Auge von Myxine 
Biolog. Untersuchg. N. F. Bd. V 1893 

2) Sanpers. Researches on the nervous system of Myxine glutinosa, 1894, 
Williams and Norgate, London. 


4 


ventralia”’, the latter of which extending ‘varying in size) from the 
entrance of the V to the X. 

In Geeenpaur’s Festschrift Fiirprincer') describes the spinal, oeci- 
pito-spinal and vagal roots (p. 616 et seq.) and gives a drawing of the 
roots of the American Myxinoid : Bdellostoma (Text figure 1). Acecord- 
ing to him the vagus leaves the brain with 1—4 rootlets (he 
draws 2) and possesses a prevailing motor character (p. 619). 

Fiirprincrr states that this also holds good for Myxine. He con- 
siders the glossopharyngeus — not mentioned by preceding authors — 
1s represented by elements of the nervus pharyngeus X, although 
he states that a branchial sack innervated by the LX is failing im 
Myxinoids. In other words he grants the absence of an independent 
IX, but supposes that elements of it are included in the pharyngeus 
branch of the X. *) 

FirBRINGuR emphasizes that the spino-occipital roots are shifted in 
a frontal direction in Myxine. This holds good as well for his 
first sensory spino-occipital root as for his second spino-oceipital 
root. The first in his opinion enters the brain on the level of 
the ramus acusticus posterior, the second near the level of the vagus 
roots. FURBRINGER points cut that, in contrast to Myxine, in: Petromyzon 
the spino-oceipital roots are located on a fairly large distance behind 
the vagus roots. 

This difference between Myxine and Petromyzon, according to 
him, can be explained in two ways, either the first spino-occipital 
root of Myxine is lacking in Petromyzon, or the spino-oceipital 
roots are shifted forward in Myxine. Firprincer believes that the 


') FiirBprineer, Ueber die spino-occipitalen Nerven der Selachier und Holoce- 
phalen und ihre vergleichende Morphologie. lestschrift fiir Gge@znBAuR Teil IIL 1897 
p. 249-766. 

We do not deal here with the paper of Ransom and p’Arcy THompson (quoted 
by Fiirsrincer) because it contains very little on our subject. Compare: On the 
spinal and visceral nerves ef Cyclostomata. Zodlogischer Anzeiger No. IX, 1886 
p. 421. 

*) We may add here that Miss WortHinGTon, to whom we owe such an excellent 
series of papers on the American Myxinoid Bdellostoma, considers this branch as 
a real IX (I. ¢ p. 172), “lying so close to the X that it is difficult to distinguish 
one from the other’. She also mentions that they have a common foramen and 
that (p. 173) “the glossopharyngeus runs in the same sheath with the vagus as 
far as the second branchial arch”. Consequently — as far as these points are 
concerning — the presence of a real glossopharyngeus is not very conspicuous either 
in Bdellostoma nor in Myxine — Since its periferal territory also is fairly well 
alrophied — (see the following pages) these arguments for the presence of a IX 
seem to be open to criticism, though in a very rudimentary way it may be 
present. 


o 
first is true, and that consequently the first sensory spino-occipital 
root of Myxine is lacking in the Lamprey. 

We may remark here that, in our opinion, FirBriNcer is mistaken 
when he considers the first root here mentioned as being a spino- 
occipital one. We are more inclined to believe that in Myxine the 
same relation is found asin Bdellostoma, for which Miss Worrninaron 
has pointed out that Firericer’s first spino-oce. root is the Acusticus 
b, i.e. a lateralis root. *) 

The topographical difference in the spino-occipital roots between 
Myxine and Petromyzon consequently is not so considerable as Fiir- 
BRINGER thought, since the spino-oecipital roots of Myxine do not 
reach as far frontally as the acusticus. 

Still there is a conspicuous frontai displacement of spino-occipital 
elements in Myxine, as appears from a comparison of Fig. 2 with 
Fig. 1. In our opinion the transitory region between oblongata 
and cervical cord is shifted in a frontal direction. 

The vago-spino-occipital region of the oblongata has approached 
the trigemino-facial region, the otic and postotie part of the bulb 
being reduced. This frontal shifting of the vago-spino-occipital region 
of the brain is acecompaniéd by a frontal displacement of the spino- 
occipital nucleus and roots, but the vagusroots (see fig. 2) are not 
so much displaced as their nucleus and remain behind, perhaps 
on account of their lying on the ear capsula. 

In consequence the spino-occipital and vagus roots have consider- 
ably approached and the vagusroots appear crowded together on the 
level of the caudal extremity of the nucleus, instead of being divided 
fairly regularly over the level of the whole nucleus as is the ease 
in Petromyzon. 

That the whole vago-spino-occipital region of the bulb has shifted 
frontally and not only the spino-occipital region, appears from the fact 
that the spino-oceipital column does not overlap the vagal column 
in Myxine more than in Petromyzon. ‘ 

As already said, this process is accompanied, if not partly caused, 
by a reduction of the acoustic region of the brain. That the acoustico- 
lateral system in Myxinoids is not very much developed results also 
from the researches of Ayrrs and WorTHINGTON *) (see further below). 
We shall now proceed to the description of the nuclear topography 
of the bulb and discuss at the same time the paper published by 


1) Compare: Quarterly Journal of Microscopical Science Vo!. 49, 1906 p. 171 
and 175. 

2) Ayers and Worruinaron: The finer anatomy of the brain of Bdellostoma 
dombeyi I. The acustico-lateral system. American Journal of Anatomy vol. VIII, 1908. 


SS -Tl MM-lV &:8-V © VW &e-V BE-K ZZ -X- Bh Spor. 


P. ROTHIG (Berlin) and C. U. ARIENS KAPPERS (Amsterdam). Further 
contributions to our knowledge of the brain of Myxine glutinosa. 


frontal 


Nucl. X mot. 


Nucl. VII—V mot. Nucl. V mot. 
Fig 3. 


Myxine glutinosa Sagittal Section. Magn. 30 : 1. 


Nucl. V mof. 


Fig. 4. 
Myxine glutinosa Magn. 20 : 1. 


Frontal Section through the frontal part of the motor V nucleus. 


Nucl, V mot. 
Fig. 5. 


Myxine glutinosa. Magn. 20 : 1. 
Frontal Section through the middle part of the mot. V-nucl. (caudally from Fig. 4). 


Proceedings Royal Acad. Amsterdam. Vol. XVIL. 


P. ROTHIG (Berlin) and C. U. ARIENS KAPPERS (Amsterdam). Further 
contributions to our knowledge of the brain of Myxine glutinosa. 


Nucl. V-VIl mot. Nucl. V-VIl mot. 
Fig. 6. 
Myxine glutinosa. Magn. 20 : 1. 
Frontal Section through the mot. V—VIl-nucleus. 


Dorsal Spino-occipital rootfibres 


Nucl, VII mot. 
Nucl, X mot, 


Fig. 7. Fig. 8. 
Myxine glutinosa. Magn. 20: 1. Myxine glutinosa. Magn. 20: 1 
Frontal Section through the mot. Vil nucl., Frontal Section through the mot. X nucl. 
caudally from Fig. 6. 


Dorsal.Sp no-occipital rootfibres 


Nucl, X mot. ee 


é 
2 
= 
Fig 9: Fig. 10. 
Frontal Section through the Nucl. X mot. Myxine glutinosa. Magn 20:1. 
Magen. 20:1 (caudally from Fig. 8). Frontal Section through the spino 


occip. column. 


Proceedings Royal Acad. Amsterdam. Vol. X VII 


7 


Hotm') on this subject in 1902, which is certainly the best de- 
scription as yet given of the motor nuclei in Myxine glutinosa. 

Horm points out that tie motor column ef the spinal cord (comp. 
our Fig. 10) can be traced frontally in the bulb. 

Laterally from it lies the posterior extremity of what Sanpers has 
called the lateral or latero-ventral cell group (comp. our. Fig. 9). 

Hotm divides this latero-central column of the bulb, which we 
shall call the viscero-motor column, into two divisions, a frontal and 
a caudal one. 

He again divides the frontal division into two, the caudal one 
into three subdivisions. 

We can only follow him in so far as we also divide the viscero- 
motor column into two divisions (see Fig. 2 and Fig. 3) of which 
however only the frontal one is again divided into two subdivisions. 
The caudal viscero-motor division, in our Opinion, is continuous (see 
Fig. 2 and 3 nucl. X mot.) and does not exhibit subdivisions. 

Apart from this column Ho_m mentions a group of cells located 
next the ventricle in the rostral part of the oblongata from which 
he thinks that a part of the motor trigeminus originates. Another 
part of the motor trigeminus should originate from a nucleus in the 
lateral part of the oblongata on the level of the acusticus ganglion. 

The nuclei of the trigeminus thus would be located at a fairly 
great distance from each other, one lying near the ventricle, the other 
near the perifery of the bulb. (Comp. lis Fig. 20 on Plate 21: 
NeIm.N V and Nell m.N Y). 

We do no agree with this description, nor with his statements 
concerning the motor facialis. 

Also the facialis — according to HoLm’s opinion — should have two 
nuclei (i.e. p. 389) and from his description it clearly appears that 
he considers our frontal motor V nucleus as a VII nucleus, for the 
axones of this nucleus — as shown in his drawings — (Fig. 21 
Plate 21) constitute the most frontal root of the bulb. 

No doubt the two VII roots deseribed by Hom (VIIa and VI1I16) 
are V roots, since only this nerve leaves the bulb with two motor 
roots *), whereas the motor VII root is single and very small. Our 
opinion is confirmed by his description of the corresponding nuclei. 

The first Vil nucleus described by this author lies in the frontal 
part of the bulb near the perifery, and consists of large cells. His 


1) J. EF. Hotm. The finer Anatomy of the nervous system of Myxine glutinosa. 
Morpholog. Jahrbuch Bnd. 23, 1902. 

*) This separation of the motor V in two roots is only visible near the en- 
trance. Soon after it they unite. 


8 


second V nucleus according to his description is located in the caudal 
elongation of the first, is not completely separated from it and 
consists of smaller cells, which description is perfectly in accordance 
with the two V nuclei (see Fig. 8) of which the second, con- 
sisting of smaller cells and not completely separated from the frontal 
nucleus, gives also rise to the VII root. (Comp. also Fig. 4—7). 

Like Hotm we were first inclined to consider the second (caudal) 
nucleus only as a VII nucleus, but a more scrutinous examination 
of the V fibres showed that in this nucleus also the second motor V 
root found its origin. 

Summarizing we state that the motor V nuclei mentioned by 
Horm are no motor V_ nuclei, and that of the two VII nuclei 
mentioned by this author the frontal one is a pure V_ nucleus, 
whilst the caudal more parvocellular one contains root cells of 
the V and VII. 

This union of motor V cells and VII cells is in perfect harmony 
with the condition found in Petromyzon (comp. Fig 1), where the 
motor VII cells also form the caudal continuation of the V nucleus 
and are a little smaller. 

Since we only wish to deal with the motor nuclei in this de- 
scription, we shall pass the acustico-lateral system, which for the 
American Myxinoid Bdellostoma dombeyi has been so minutely 
described by Ayers and Worrnineron *) and proceed to the motor 
X nucleus of Myxine. 

It is obvious that, without an examination of the periferal nervous 
system and its muscles, the question of the presence or absence of 
a motor glossopharyngeus cannot be settled. 

We can only state that our researches show a reduction of the 
number of root fibers of the motor X group, which in Myxine only 
consists of 3 of 4 rootlets, whereas in Petromyzon it contains 
together with the glossopharyngeus at least 5 rootlets. 

This combined with the fact that the posterior visceromotor column 
has suffered a reduction in its frontal part is in harmony with the 
opinion defended by Jounsron *) that the glossopharyngeus and perhaps 
even the first motor X root sensu strictiori are either very much 
reduced or absent. A comparison of Fig. 1a and 2a shows that this 
reduction is only probable for the frontal pole of the column, 


1) Ayprs and WortHINGToN: They finer anatomy of the brain of Bdellostoma 
dombeyi. I. The acustico-lateral system. American Journal of Anatomy Vol. VIII, 
1908. 

*) Jounsron: Note on the presence or absence of the glossopharyngeal nerve 
in Myxinoids. Anatomical Record Vol. Il, 1908, 


2a. 


“u~ 
DC SOC 


Showing the reduction in the frontal part of the vagal column. 


since the overlapping of the caudal part of the vagal column and 
spino-occipital column, as well as the topography of the posterior 
extremity of the vagal column to the spino-occipital roots, are the 
same in both Petromyzon and Myxine. 

The reduction of the roots and of the frontal part of the vagal 
column in Myxine is also in harmony with Srockarpb’s observation 
that in Myxinoids, at least in its American form Bdellostoma, the 
branchial sacks behind the hyomandibular arch are atrophied. *) 

The vagal column begins fairly near the posterior extremity of 
the mixed V—VII nucleus, lying in a somewhat more dorsal position 
(Comp. Fig. 3,7 and 8). A few seattered cells lie between them, thus 
constituting a sort of broken link. 

The size of the vaguscells is considerably smaller than that of 
the frontal V nucleus, more like the cells of the mixed V—VII 
nucleus, specially the smaller caudal cells of the latter. 

In its frontal part.the vagus nucleus is rather small and the cells 
do not attain their largest size here. The nucleus as well as the 
cells attain their maximum development in the middle part. We 
have not been able however, to state a division of the nucleus in 
three parts as Hoxm did. 


1) SrockarRD: The development of the Mouth and Gills in Bdellostoma Stouti. 
American Journal of Anatomy Vol. V 1906, specially p. 511 and fig. 35—3s6. 
Compare also for further knowledge of these animals : 

Ayers. Bdellostoma dombeyi. Woodshole lectures for 1893. 

WortTHINGTON. Centribution to our knowledge of the Myxinoids. American 
Naturalist Vol. 39, 1905. 


10 


On the other hand we agree with Hotm that the small ventro- 
lateral root that leaves the bulb in the posterior part of the vagal 
region and is considered by SanpErs to be a vagalroot, is certainly 
a spino-oceipital one (Cf. Hotm p. 395), as much on account of its 
position as on account of its central connection. — 

That the spino-occipital column extends for a short distance in 
the vagal region is a general feature in vertebrates and has been 
shown before to occur also in Myxine by Epinerr *) (I. ¢. p. 28). 

We also agree with Hoim that the dorsal sensory root entering on . 
this level is a sensory spino-occipital or spinal root and not a sensory 
Vagusroot, as results from the facts 1. that the size of its fibres 
corresponds with those of the sensory spinal rootfibres, 2. that the 
line of entrance and the ascending character of the fibres during 
their intramedullary course are the same as in the spinal sensory 
roots and 3. because they are joined by the latter during this 
course. 

Finally we wish to call attention to the fact that not only the 
topography of the uuelei, but also the general morphology of this 
brain shows the compression which the brain has suffered. 

Similar to the other ventricles of the brain the 4" ventricle is 
reduced to a minimum. This is complicated by the peculiarity that 
the caudal end of the midbrain (a cerebellum does not occur in this 
animal) protrudes a considerable distance between the dorsolateral 
walls of the oblongata and is so closely adjacent to it that ouly the 
pial membrane can follow it. Behind the caudal extremity of the 
midbrain the dorsolateral walls of the oblongata unite. 

One cannot speak here of a real calamus scriptorius caused by a 
widening of the ventricie itself. The lateral deviation of the walls 
takes place only under the influence of the midbrain, but the 4t 
ventricle itself remains a small split underneath it. The dotted arrow 
in figure 2 indicates the place of this pseudo-calamus. Since in this 
animal, with atrophic eyes, there is no question of an enlargement 
of the midbrain being the cause of this telescoping, the only reason 
of it can be found in the compression of the whole brain in its 
longitudinal axis, which is also exhibited by the approach of the 
vago-occipital part of the oblongata to the trigemino-facial part. 

This longitudinal compression probably finds its chief reason in 
the pressure exercised on the frontal part of the brain by the 
olfactory pit and dorsal lip, the influence of which on the form 

1) Epryaur: Das Gehirn von Myxine glutinosa. Abhandlungen der Preussischen 
Akademie der Wiss. 1906. 


11 ‘ 


of the brain in Cyclostomes is already mentioned by Scorr ‘) in 
Petromyzon. 

As stated above, the telescoping is the more obvious in the 
oblongata on account of the reduction in the acustico-lateral system 
of the bulb. 

Everything indeed shows that in Myxine we have to do with 
considerable secondary modifications. 

Also the topography of the motor nuclei is by no means a primi- 
tive one. 

The primitive location of the V, VII, and X nuclei in Cyclostomes 
is near the ventricular ependyma where the matrix of the nerve 
cells is, and where they are still found in Petromyzon. In Myxine, 
however, the V—VII nucleus has a ventro-lateral periferal position 
and the X nucleus a lateral periferal position, a condition that can 
only be caused by secondary influences originating in the functional 
reflectory relations of this animal. 

The influence which has caused this secondary position is certainly 
the considerable development of the descending sensory V, which 
has a dominating influence on the structures of the oblongata, an 
influence which is the more prevailing since the other sensory and 
reflectory paths are either atrophied or poorly developed in this 
animal. We know that in animals with a well-developed dorsal 
viscero-sensory nucleus the motor vagal column generally has a 
dorsal position, adjacent to its sensory grey (Selachians), which is 
still the case even in Petromyzon. 

On account of these facts we cannot agree with Hotm in his 
statement that Myxine has a more primitive character than Petro- 
myzon. 

Summarizing our results we conclude : 

In Myxine the eye-muscle nuclei are absent. 

The motor V nucleus is incompletely divided into two parts corce- 
sponding to the central division of the motor root into two parts. 

In the continuation of the caudal V nucleus also the motor VII 
cells are found, as is also the case in Petromyzon. These nuclei have 
a ventrolateral position very near the concomitating grey substance 
of the sensory root. A central V nucleus (Hotm) has not been found. 

The posterior viscero-motor column, and also the spino-occipital 
motor column has shifted considerably frontally. By the adjacency 
of the earecapsule this shifting could only be partly followed, by 
the motor X roots, which are crowded together on the earcapsula. 


') Scorr. The embryology of Petromyzon. Journal of Morphology Vol. 1, 1887 


12 


The spino-oceipital roots have, however, followed the shifting of their 
nucleus and have come very near the vagus roots. 

The posterior viscero-motor column is considerably shortened at 
its frontal extremity, which most probably results from the 
absence or extreme reduction of the motor IX, and perhaps even 
of the frontal motor X root (JOHNSTON) in connection with the absence 
or reduction of the two posthyomandibular branchial sacks (Stock aRD). 


Physics. — “Further experiments with liquid helium. J. The imitation 
of an Ampbee molecular current or of a permanent magnet by 
means of a supra-conductor.” Communication N°. 1046 from the 
Physical Laboratory at Leiden. By Prof. H. KamErtinen OnnEs. 


(Communicated in the meeting of April 24, 1914). 


§ 1. lntroduction. If a current is generated in a closed supracon- 
ductor, from which no other work is required than what is necessary 
to overcome the possible remaining micro-residual resistance of the 
conductor, it follows, from the small value that the micro-residual 
resistance can have at the most, that the current will continue 
for a considerable time after the electromotive force that set it in 
motion has ceased to work. The time of relaxation + in which 
the current decreases to e-!t of its value is given by the ratio 

of the self-induction Z and the resistance 7 of the circuit. When 
s 
r approaches zero, this period may rise to very high values. Whereas 
the time of relaxation is extremely small in ordinary cases (for the 
coil with which we are about to deal for instance, of the order of 
a hundredthousandth of a second) when the resistance in the supra- 
conducting condition becomes say 1,000,000 or even 1,000,000,000 
times smaller it may increase so much, that the disappearance of 
the current can be observed ; it may even take place extremely slowly. 

From the moment that [ had found in mercury a supra-conductor 
at the lower temperatures which can be obtained with liquid helium, 
I was desirous to demonstrate the persistence of a current in a con- 
ductor of this kind, and amongst other things to take advantage of 
it in the further investigation of the microresidual resistance of the 
supra-conductor '). But it was only after the previous study of various 

1) For the sake of brevily we use the word resistance here in the sense of 
quotient of potential difference and current strength. In supra-conductors (see 
Comm. No. 133) we can at present only speak of current and potential difference ; 
whether the relation between these two can be expressed by means of the concep- 
tion of specific resistance, has still to be investigated. (Comp. note 1 § 3), 


13 


problems, which were also of value for the knowledge of the con- 
ditions which had to be considered, that I arrived at the simple 
experiment which I am now able to deseribe, and whieh confirms 
what I have adduced in a convincing way. 

For this experiment a conductor was available whose constants, 
in so far as they were needed in designing the experiment, were 
known: I refer to the coil of lead wire Phx which has several 
times been mentioned in previous papers. A thousand turns of lead 
wire of ‘/,, sq. mm. in section are wound on a small brass tube 
of 8 mm. in diameter in a layer 1.1 em. thick and 1.1 em. lone. 
At the ordinary temperature the coil has a resistance of 734 2 and 
as the inductance is I milli-henries, the relaxation time may be put 
at about 1: 70000 of a second. The micro-residual resistance at 1°.8 Kk. 
had been found to be more than 2 > 10°° times smaller than the 
resistance at the ordinary temperature ; the relaxation time therefore 
must be at least of the order of a day. The limit to which the current 
may be raised before ordinary resistance is suddenly generated, had 
also been determined ; at 1°.8 K. this limit was 0.8 amp.; it is clear 
that a lower current than that is sufficient to make the coil into a 
powerful little magnet. Finally the threshold value of the magnetic 
field, below which no resistance is produced in the coil was known : 
at 1°.8 K. it had been found to be about 1000 gauss. It was ascer- 
tained (ef. § 3), that if was unnecessary to use a field of that strength 
to be able to make the experiment by means of generating a current 
by induction in the conductor. The conductor after having been tested 
as to its superconductivity had to be closed in itself in a supereon- 
duetive way. This was effected by fusing the ends of the lead wire 
together: in previous experiments it had been found, that this treat- 
ment did not lead to the production of ordinary resistance. In view 
of all the data I could be assured, that all the conditions necessary 
for the suecess of the experiment were fulfilled. 


§ 2. Arrangement of the experiment. The coil was fitted up in 
the same eryostat which had served for the previous experiments 
with the plane of the windings vertieal in such a manner, that it 
could be raised and lowered, as well as turned round a vertical 
axis. Fig. 1 shows the arrangement diagrammatically. 

As the coil was closed the current in it was generated by induction. 
A large Wuiss-electromagnet, at hand for the experiments of Comm. 
N". 140d could be moved on casters towards the cryostat to a position 
in which the cryostat with the coil was in the interferrum, 

In order to obtain an unambiguous result it is advisable to be 


14 


able to test the magnetic condition of the coil while no other magneti¢e 
objects are in the neighbourhood; it is also necessary to prevent the 
induction currents which are generated when the field is produced 
and when it disappears from partly or completely neutralising each 
other (cf. § 4). . 

It can therefore be easily seen that the follow- 
ope ing procedure is advisable: the field is put on, 
while the coil is in the cryostat at the centre of 
- the interferrum, everything being prepared for 
|| siphoning the liquid helium into the eryostat. 
| The current generated at the production of the 
field is then immediately dissipated by the ordinary 


| | resistance of the coi before the helium is poured 
over. Care is taken to keep the field below the 
threshold-value of the production of ordinary 
resistance, which holds for the temperature at 
which the experiment is going to be made. The 
coil is then cooled by letting in liquid helinm, 
the field remaining unchanged. In this manner a 
supra-conducting coil is obtained, closed in itself 
- without a current placed in the magnetic field. 
If the field is now put off and the apparatus 
which have produced it are removed, a current 


a will remain in the coil which is smaller than or 
in the limit equal to the threshold-value corre- 
sponding to the temperature of the coil. The presence of this current 
can be established by its magnetic action outside the cryostat. 

In order to obtain a strong current it is advisable te cool the 
coil as far down as possible, as thereby the threshold-value of the field 
to be used for the induction and the threshold-value of the current 
are both made as high as possible. Fer that reason the first experiment 
was made at a temperature of 1°.8 kK, the towest temperature which 
can be reached comparatively easily and maintained for a long time. 

§ 3. Culeulation of the experiment. Assuming that the field 
diminishes proportionally to the time ¢ from //, to O and ealling J/ 
the magnetic potential of the coil in the field //, “will be constant 


during the period of the disappearance of the field and the equation’) 


!) Here is supposed that 7 is independent of 7 below the threshold value ip of 7. 


15 


with 70 at the beginning gives 


1 dM — 3 
EAM bites ). 
r dt 


‘i 
and for small values. of and ?¢, as lone as J/ has not reached 


zero, With sufficient: approximation 
| 1 aM 


= (Fe) 
Ts it 


so that, if M/ reaches O while ¢ is still small, 


will be the final value of the current. 

In our experiment the constants were //, = 400, J/,= 1,26 10°, 
L=10', so that 2 could rise to 0,126 C.G.S. or 1.261) Amps. 
The current can therefore reach the threshold-value 0.5 Amp. even 
with a field of rather more than half the strength assumed in the 
caleulation (cf. one of the experiments in § 4). From the moment 
at whieh this value is reached ordinary resistance appears and i 
will be no longer small; the further increase of 7 above the threshold 
value zp follows a different law from below 7p. 

For an aecurate calculation of the process above 7p, it would 
be neeessary to take into account the complicated law of imerease 
of the resistance with the current beyond 7p. For our purpose it 
is sufficiently accurate to assume, that when 7p is exceeded by a 
small amount, the resistance becomes suddenly 7 of the order of 
magnitude above the vanishing point. 


dM .e 
In that case, a remaining the same as before, the current will 
aL 
aw \duw 
be able to rise by a small amount ¢—ip = — a whieh will soon 
yr 


dM 
be reached, will then become constant and, on J/ and ar becoming 
td 


zero, disappear again in a short time. In view of the value of J/ 
and r’ we may, if J/ does not change very rapidly, disregard <—7p, 
unless we intend an explanation of all the details of the experiment, 

We therefore come to the conclusion, that, J/, being sufficiently 


') The more accurate data given here differ somewhat from those in the Duteh 
text. 


16 


large, the current (Fig. 2) on M diminishing to O will reach the 
threshold-value, belonging to the temperature of the experiment, and 


mp 


m 


by 


Fig 2. Fig. 3. 


after the induction being completed will continue, while only after 
a long time /# according to the relation 


in accordance with the large value of the time of relaxation — 
T 


an appreciable diminution of 7 will be observed. 

The ease, that the initial value of J/ is above the threshold-value 
of the production of resistance Mp, is represented in Fig. 3, which 
after the foregoing needs no special elucidation. The result is ap- 
parently again dependent on the threshold-value of the current (see 
also one of the experiments in § 4). 

As appears from the values given above an initial field much 
smaller than J/, was sufficient in our experiment. 

According to the above calculation it was to be expected, that 
the examination of the magnetic action of the coil could be per- 
formed with a simple compass-needle broughi near the eryostat. 


§ 4. Details of the observations. The result proved the correctness 
of the discussion contained in the previous sections. The field was 
taken at 400 gauss. In 10 seconds it was reduced to 200 gauss 
and immediately afterwards the electromagnet was rolled away in 
5 seconds. The compass-needle which was then placed beside the 
cryostat to the East of it on a level with the coil and ata distance 


17 


from it of 8 ems pointed almost at right angles') to the meridian. 
When the action on the magnet was compensated by means of a 
second coil placed on the other side (West) of it of about the same 
dimensions as the experimental coil and of 800 turns, it was found 
that the coil was carrying a current of about 0.5 to 0.6 amp. *). 
This was further confirmed by turning the coil and by moving the 
compass-needle to various positions about the cryostat *). During an 
hour the current was observed not to decrease perceptibly (as far 
as could be judged by the deviation of the needle with an accuracy 
of 10°/,). During the last half hour the coil was no longer at 
1°.8 Kk. but at 4°.25 K. the temperature of helium boiling under normal 
atmospheric pressure. Undoubtedly even at this temperature the 
observation might bave been continued much longer without much 
diminution of the current. A coil cooled in liquid helium and provided 
with current at Leiden, might, if kept immersed in liquid helium, 
be conveyed to a considerable distance and there be used to demon- 
strate the permanent magnetic action of a supra-conductor carrying a 
current. | should have liked to show the phenomenon in this meeting 
(Kon. Acad. Amsterdam), in the same way as I brought liquid 
hydrogen here in 1906, but the appliances at my disposal do not 
yet allow the transportation of liquid helium. 

Whereas the experiment, so far as described, shows, that a current 
when started in a supra-conducting wire continues to flow, the 
process is immediately stopped as soon as ordinary resistance is 
generated in the circuit. When the coil is lifted out of the helium, 
the current is instantaneously destroyed. The temperature of the 
coil is thereby very quickly raised above the vanishing point of 
lead (6° K) and the very long relaxation-time is replaced by a very 
short one. Reimmersion of the coil, if not too soon after the lifting 
out, does not again produce magnetic action. 

If the experiment is made with the windings of the coil parallel 
to the field, no effect *) is to be expected. This expectation was in so 
far confirmed as only a slight effect was observed: this effect cau 


1) The field of the earth being distorted by machinery the action of the latter 
was compensated by magnets and there resulted a weaker field (note added in 
the translation.) 

2) [Calculated from the moment, comp. N®. 140d § 8, end. Added in the trans- 
lation}. The coil has a magnelic moment of about 180 C.G.S. and behaves as if the 
lead possessed remanent magnetisation of some 200 C.G.S. units. 

8) On repeating the experiment at 4°.25 K. nearly 0.5 amp. was obtained; a 
later experiment with larger initial field at 2°.3 K. gave 0.7 amp. (see further down). 

') Nearer consideration points to a small effect Comp. N°. 140c (Note added in 
the translation). 


Proceedings Royal Acad. Amsterdam. Vol. X VIL. 


18 


be sufficiently explained by assuming that the attempt to place the 
windings exactly parallel to the field had not sueceeded. *) 

If the initial value of the field is higher than the threshold-value, 
Mp the result is the same. Tlus case is represented in fig. 3. In 
one experiment the initial field was 5000 gauss and the observed 
magnetic moment corresponded to a current ¢ = 0.7 amp. 

If the field through the supraconducting coil is first put on and 
subsequently put off again by bringing the excited electromagnet 
to its position at the cryostat and then removing it, according to 
the above reasoning (disregarding the exceedingly slow diminution 
with the time) no resultant current ought to remain, if no account 
had to be taken of the threshold-value of the current. Indeed for 
Gre Sa! gale ; : 
the second period the relation 7—7,e ° = a holds, if ZL is 


4 


7 the current obtained in the 
) 3 5 . 
3 first period during the gene- 


ration of J/,. This case will 
be realized, if care is taken, 
that the threshold-value of 
-ig fa -==--b == 7 ~- = the current is not exceeded. 
7 It is represented in fig. 4 
by the lines which give the 
field J/5 and the current 


7, as funetions of the time. 
If during the increase of 


M = the threshold-eurrent is 
reached, the current will not 


grow appreciably on further 


Fig. 4. 


rise of J/; from the moment, 
that the inerease of J/ stops, the current assumes the threshold-value 
and stays there, until J/ begins to decrease: it then begins to fall 
and becomes zero, before the field has disappeared; on the further 
diminution of the field, the current assumes the opposite sign and 
the resultant current will be that whieh has been formed at the 
moment that J/=0, if it remains below the threshold-value, or the 
threshold-current itself, if that is reached before J/ has disappeared. 
In the latter case the current will exceed the threshold-value by 

') This expériment had been made some says before the main experiment, although 
it had not been the intention to make it with that position of the coil. So far it 
has not been repeated. At the moment of making this first communication it had 
not been repeated. [It has been repeated since; again a rest was found, (Note 
added in the translation. Comp, Gomm. N°. 140c)]. 


19 


a very small amount from the moment, that the threshold-value is 
reached, until J/ = 0. In fig. 4 this case is represented by the lines 
which give the relation between the field J/, and the current Za. 

An instance of the case represented by a is given by an experi- 
ment, in which the field brought to the eryostat was 400 gauss. A 
strong resultant current was observed as in the ease, when the coil 
was first free of current in the field of 400, was then made supra- 
conductive and was finally charged with current by the removal of 
the field. An instance approximately corresponding to case was 
obtained, when the same experiment as @ was carried out with a field of 
190 gauss. Even in this case the compensation was not quite complete 
and a little more favourable. when the field was made to approach 
slowly, than with a rapid approach. 

With a rising field account has to be taken also of the compli- 
cation arising out of the influence of the field of the current itself on 
the threshold-values of the field and current. In fact this was not the 
only feature in the experiments which could not be fully explained 
yet: naturally as they were performed for the first time, the arrange- 
ments were still imperfect '). Taken together however they may be 
said to confirm the main experiment which shows that it is possible 
in a conductor without electromotive force or leads from outside *) 
to maintain a current permanently and thus approximately to imitate 
a permanent magnet or better a molecular current as imagined by 
AMPERE. 

The electrons once set in motion in the conductor continue their 
course practically undisturbed, the electrokinetic energy, represented 
by Maxwet1 by the mechanism of the rotating masses coupled to 
the current, retains its value, the rotating fly-wheels go on with 
their velocities unchanged, as long as no other than supraconductors 
come into play: the application of a small ordinary resistance 
however stops the mechanism instantaneously. Although the experi- 
ment mainly confirmed my deductions as to what had to be expected, 


1) One of the first questions still to be answered is, what part a possible magnetisation 
of lead or brass may have played in the phenomena: so far no proof las been 
given, that this may be neglected. However, even now from the experiment, in 
which the windings were parallel to the lines of force, we may draw the conclusion, 
in view of the small amount of the action in that case, that the magnetisation 
of the material of the coil can only play a very subordinate part compared to the 
electromagnetism of the current, to which I have above ascribed the deviation of 
the compass-needle. 

*) It may be mentioned here, that it will be possible, by a change of tempera- 
ture of a small part of the conductor, to insert a resistance in the circuit which 
can be very delicately regulated without touching it. 

)%* 


20 


a deep impression is made by the very striking realisation which 
it gives of the mechanism imagined by MaxwrLi completed by the 
conception of electrons. 

It is obvious that the subject will lead to further discussions *) 
and plans, but in this paper 1 may be allowed to confine myself to 
the simple description of the experiment carried out. 


Physics. — “The chemical constant and the application of the 
quantum-theory by the method of the natural vibrations to the 
equation of state of an ideal monatomic gas.’ By Dr. W. 


10 


H. Kuvsom. Supplement N°. 364 to the Communications from 
the Physical Laboratory at Leiden. (Communicated by Prof. — 


H. IK AMERLINGH ONNws). - 


(Communicated in the meeting of March 28, 1914). 


§ 1. In Suppl. N°. 33 (Dee. 1913) the expression for the entropy, 
S, of a gas was discussed, as it follows from the application of the 
quantum-theory to the molecular translatory motion by the method 
of the natural vibrations. Molecular rotations and intramolecular 
motions were not taken into account there. As was observed, the 
chemical constant is connected with the additive constant which 
occurs in the development of S for high temperatures. The object 
of this paper is to show that the value of the chemical constant, 
which in that manner is deduced from the expression for the entropy 
(an expression which had already been given by Trrropg), is in 
satisfactory agreement with values of this constant which correspond 
to the experimental data concerning vapour pressures of monatomic 


OAcaS 
gases. 


§ 2. We shall confine ourselves in this paper to the consideration 
of monatomic gases. If for the energy distribution one of the tem- 
perature functions is assumed which occur in the quantum-theory, 
one may suppose that the molecular rotatory motion, particularly 
for the molecules of a monatomic gas, is in thermal equilibrium 
say with the translatory motion. If in particular that temperature 
function (given by Pranck) is assumed which implies a zero point 
energy, the molecular rotations in a monatomic gas also, at the 
temperatures at which they have been investigated, represent a con- 
siderable amount of energy in proportion to the molecular trans- 


1) Compare also MAXWELL, Electricity and Magnetism Il, Ch. VL. 


21 


latory motions. The characteristic temperatures (@,, ef. Suppl. N°. 382), 
which according to that hypothesis govern the rotatory energy, are, 
however, owing to the small moment of inertia of the monatomic 
molecules, so high, that at the temperatures mentioned the energy 
of rotation of the molecules does not yet deviate appreciably from 
the corresponding zero point energy. The same applies to the motions 
within the atom. The contributions to the entropy due to these 
rotations of and motions within the atom may then be counted as 
zero. We limit ourselves to the temperature range within which this 
is the case’). 

We shall further assume that we are dealing with an cdeal 
monatomic gas, so that terms due to the influence of the real 
volume or of the mutual attraction of the molecules need not to be 
considered. 

The entropy of such a gas is then, on the basis of the hypot 
of Suppl. N°. 30a, determined by the expressions given in Suppl. 


N°. 33 § 2a. 


heses 


Q 


§ 3. In the first place, as was already observed in Suppl. N°. 33 
§ 2af8, the introduction of the zero point energy makes no change 
in the value which is found for the chemical constant. Hence a 
comparison of the value calculated for this constant, e.g. with the 
value which was found by Sackur to agree with experimental data, 
cannot furnish a test between PLANck’s formula with or without 
zero point energy ’*). 


§ 4. If the development of S for high temperatures: equation (14) 
Suppl. N°. 338, is written in the form 


S=C,4+ Nklnv + */, NklnT + 


1 
-+ terms of smaller order of magnitude () 

then 
C= Na(4 a Ina), Tera ees (2 


1) According to measurements by Pier of the specific heat of argon, this tem- 
perature range extends for this gas to at least 2300° C. As Prof. Euysrein pointed 
out in a discussion, the investigation at high temperatures of the specific heat of 
a monatomic gas with high atomic weight, such as mercury, would be of great 
interest. 

2) Prof. SOMMERFELD asks me to say, that he wishes the sentence: “Nebenbei 
sei bemerkt etc. on p. 139 of: Vortriige tiber die kinetische Theorie der Materie 
und der Elektrizitét,’” Leipzig und Berlin 1913, to be omitted. 


22 


From equation (13) of Suppl N°. 83 with equation (187) of Suppl. 
N’, 30a it follows that 


3k? (42 7s 
(= saa (Gx) oh Oe re 
Krom these formulae. follows for the entropy constant 
C, = NE 4 a eee (aa) {- oo, ul On Re 
9 Nh? \5Nk 


With the values V = 6.85.10** (according to Perrin), 4 = 1.21.10 1°, 
h 


kh 
(4) with WA = PR passes into 


= 4.86.10°"', which were accepted in Suppl. N°. 30a, equation 


0, =n |= in M— 7.48) . se Sees 


If we take MiiiKan’s?) values V=6.06 .107, £=1.87 .10-“, 
h 
; — 183.107 "", we find 


M — 7.285 (5b) 


| 


For the chemical constant Cyp, which is derived from C, by 
means of the relation *) 
é C, — 2.5R + R In Nk 
CAS ae Rint 


we find 


Oni = log M +- 3.60 Pee) el ee (6a) 


and in ¢.g.s. units 


Crus = 5 log M + seal SE SG (60) 


respectively. 

These values differ from those which Sackur has compared with 
the vapour pressures of mercury and argon and which he found 
fairly well confirmed, only by 0.85 and 0.28 respectively. This 
agreement may be called very satisfactory considering the uncertainty 
which yet exists with regard to several of the quantities used in 
that comparison on the one hand, and the approximate character of 
some of the hypotheses on which the deduction of the expression 
for the eninopy was founded on the other hand. 


1) ne aa Miuurkan, Physik. ZS. 14 (1913), p. 796. 
2) Gf. O. Sackur, Ann. d. Phys. (4) 40 (1913), p. 


23 


§ 5. The relation (4) also follows from equation (19a) of the 
paper by SommurreLp (p. 134), quoted in note 2 p. 21, if@ occurring 


10 
there is put equal to ioe as has been supposed in the relations (3) 


and (4) given above, and if in SomMmrrELD’s expression /: is replaced 
by 4 A'). The latter change is connected with the fact, that in 
deriving the expressions given here the supposition was made that 
in considering the molecular translatory motion in an ideal monatomic 
gas we have to deal with energy elements of a magnitude } hy, as 
we tried to make probable in Suppl. N°, 30a § 2. 

The fact that in § 4 a satisfactory agreement with experimental 
data was obtained, may, if the validity of the other hypotheses is 
admitted as sufficiently approximate, be regarded as a confirmation 
of the above supposition concerning the magnitude of the energy 
elements. 


Astronomy. — “On Sevnicer’s hypothesis about the anomalies in 
the motion of the inner planets.” By J. Wourinr Jr. (Com- 
municated by Prof. W. pe Srrrer). 


(Communicated in the meeting of April 24, 1914). 


To explain the differences between observation and calculation in 
the secular perturbations of the elements of the four inner planets, 
SEELIGER *) worked out the hypothesis that these are caused by masses 
of matter, which by reflection of sunlight offer the aspect of the 
zodiacal light. He imagines these masses to have the form of a flat 
dise surrounding the sun and extending nearly in the direction of 
the orbital planes of the planets and reaching outside the orbit of 
the earth; the density of the matter within the dise has its greatest 
value in the proximity of the sun, though it is very small even there. 
For the calculation of the attraction of the mass of matter special 
hypotheses on its constitution are introduced; we imagine a number 
of very flattened ellipsoids of revolution with the sun at the centre, 
the inclinations of the equatorial planes to the orbital planes of the 
planets being small. It is evident that by the superposition of a number 
of such ellipsoids we get a flat dise within which the density varies 

1) This confirms at the same time the fact, that the introduction of the zero 
point energy does not produce a change in the value of the entropy constant. 

2) Das Zodiakallicht und die empirischen Glieder in der Bewegung der innern 
Planeten, Sitzungsberichte der Bayerischen Akademie, XXXVI 1906, 


24 


after a certain law from the centre outwards. SeenigEr arrived at 
the conelusion that two ellipsoids suffice, one of which is wholly 
contained within the orbit of Mercury, the other reaching outside 
the orbit of the earth. There appears to exist a certain liberty in 
choosing the values of the ellipticities and the quantities determining 
the position of the second ellipsoid. As quantities to be determined 
so as to account for the differences which are to be explained 
SrvLiceR introduces the densities of both ellipsoids, the inclination 
and the longitude of the ascending node of the equatorial plane of the 
first ellipsoid with reference to the ecliptic, and a quantity not con- 
nected with the attraction of the masses of matter, but relatiug to 
the deviation of the system of coordinates used in astronomy from 
a so called “inertial system”. 

Last year Prof. py Sirrek drew my attention to the necessity 
of festing Sepiicer’s hypothesis by calculating the influence of the 
masses admitted by Seeriger on the motion of the moon and the 
perturbation of the obliquity of the ecliptic, which Srerierr did not 
consider’). | performed the calculations and arrived at the conclusion 
that the perturbation of the ecliptic changes the sign of Nswcomp’s’) 
residual and makes its absolute value a little larger; further that 
the perturbations of the motion of the moon are insensible. I may 
be allowed to thank Prof. pr Srrrer for the introduction into this 
subject and the interest shown in its further development. — One could 
take the formulae required for the last mentioned purpose from 
Surnicur’s publication; I did not do so, but developed them anew. 
I give them here on account of small differences in derivation. First 
I shall give this derivation and the results; after that I shall do 
ihe same for the motion of the moon. 


I. Perturbations of the ecliptic. 

Let x,y,z be coordinates in a system the origin of which is at 
the centre of the ellipsoid, while the axis of rotation is the axis of 
z, kh? the constant of attraction, g the density of the ellipsoid, a, a 
and ¢ its axes, then the potential V at the point w, y,z is given 
by the expression : 


f= barge | 1.— = == ———y 
‘ Vtu c+u/) (a+tuwye +u 


1) See pe Sirrer, the secular variations of the elements of the four inner 
planets, Observatory, July 1913. 
2) Astronomical Constants p. 110, 


No 
ur 


for a point outside the ellipsoid 4 is the positive root of the equation 


vty? ae P 
qa ee = 0; for a point inside A is zero. 
ata c aE 

Z* 77 we have: 


Putting V = k’nqa’c2 and #+y?'+2=r 


ae > 1 rT z*(a?—c’) du 
ae, =| ( atu “Sass, (7+ SE ana a 
" aa’ —c*) 


Ta) Gea) 


Perturbations caused by the jirst ellipsoid. 
I develop in powers of 27 =, § being a small quantity ; for that 


purpose we need (neglecting terms of the third order) : 


(= Ey An of du ks 
OS) hae (a* (a? +-u)? (c? +u)'l2 


r—a* 


?Q Pe (a?—c’)? 
0c? es r(r?—a? + cy ile : 


I put r=a,(1+ 8) and develop the part of $2 independent of 
$ besides the coefficients of the different powers of § in powers of § 


Introducing the quantities : 


o.=f- = du C of du 
(a? +- eae @+ wu)” Vay : (a° + w)*(c? --u)"h 
a,*—a* ;2—a? a,?—a? 
a 2 A oe} a," —= 
a*— a’+c=p ax 7 
we get 
>) y 5° 2 2 3° 
2=C,—4/C, — str@rerarG) Oh —gats tile 
1 1 1 NES _v—c* eA Anes A eas 
aMGachia Yate ach 6 Cee pp ost (- 9 —3y)s + 
2 2 P a,"p 
Per z 27 1) SOLE Ns 
ae (Esa On ae Wace ar i= a a a ag ee 8 sla 
1 JG Cu)a 
bh 
2 Co Ie 


Let v be the true anomaly of the planet, y the angular distance 
between the ascending node of the equatorial plane of the ellipsoid 
on the orbital plane of the planet and the perihelion of the orbit 


26 


J ihe inclination of the equatorial plane to the orbital plane, then 
we have 
z= — a, (14+ §)sin(v + W) sin J 
S=a,?(1 4 §)? sin? (v + wy) sin? J. 

For the ecaleulation of the secular portion of the perturbative 
function we thus need the secular portions of §”, §? sin? (v + yw) and 
sin'(v-+ wp) for different values of p. I get (denoting the secular 


| 


portion by the letter S): 


mt é 4 é? Aye 3 bs 3 
co Si 5 SS re Se 
sin? (v + w) =~ — Ge + gt ore 
8 6 
§ sin® +m = pe(1—perrw) + Georre 
2 


1 1 1 
S § sin? (v + yw) = rn é? (: — 5 008 2 v) =6 e* cos 2 wy 
@ za 3 1 A 
538 , =— i — 0) S Z 
S §* sin? (v + w) = e* 6 are cos 2 W 


3 1 
S § sin? (v + pw) = e* ae: 


a 


S sin’ (v + py) = 


Substituting in the expression for £2 we find : 


ae e? 3 ee ée 1 1 ome 
Soars ae ae e ace ) > ( io. 6a aa 


P a 
: v—ec oe i 1 a A A 3 3 3 aa 
| at sin? J 15) Ci ap +e To ae Y— i C,a,7p* + 
v 3 5 j ‘ ae 9 ee) 
tyr CO8 SDI agate pn sae aa gat t+ go? 


105 


1 ee 3 25 35 ‘| 3 (w@’—c?)? ip 
= cos2y | — = 4 
rie tn 39° ral Tete a sin 


Let 7, © and § be the inclination, the Ne: of the perihelion 
and the longitude of the ascending node of the orbital plane of the 
planet, /, and ® the inclination and the longitude of the node of 
the equatorial plane of the ellipsoid all with reference to a fixed 
fundamental plane, e.g. the ecliptic of a certain epoch ; then we have: 

sin J cos (W-— w + 9) = — cos J, sini -} sin J, cos i cos (§4 — P) 


sin J sin(w — & + QQ) = sin (84 — &) sin J. 


27 


E ; Ad Ee ; 0S OJ Ow Oy, 

From these expressions we can determine ag a Ope i the 
quantities required for the computation of the derivatives of 2 with 
regard to these elements. In view of the calculation of the perturbation 
of the obliquity of the ecliptic I do not use the elements 7 and {), 


but the elements p and gq thus defined : 


p=tanisin §% 7 = tani cos §% 
I get: 
ay Z ale 2, Seat) ) 
— = cost | cos? — sin (yw -— @) + sin? — sin (w — wo + 2Q) 
Op 2 2 { 
Oc 
ca ae 3? = e083 (wy — @) — sin* = cos ( — @ + 29) 
q 
Ow 
Shae =sin Ftan © eosieos Qt cosJeosi cos + cosy )-+sin? “ cos(tp- 0+29)) \ 
P 
mee, Pt ee Ree eerie aay eee See 
stn. eae tan Sie aac! cost} cos ee SO) ae 5 eintp-O+ 28) ; 
The differential equations for p and q are’): 
dp _ 1 OV 
dt na,2V 1—e*cos*i 99 
dq l OV 
dt na,*V 1—e’?cos*i Op 


To verify these formulae I have used them for the computation 
of some of the perturbations of 7 and §), which are given by 
SEELIGER °). 

To compute the perturbation of the obliquity of the ecliptic I take: 

Sued 


V = — k*xqa’e (a*—c’) C,a,’ 


According to SeeiicEr’s data a= 0.2400, c = 0.0239, J=6°57'.0 
I get C,=0.426; taking as unit of mass the mass of the sun, as 


unit of time the mean solar day I get log ¢ = 0.7119 — 5 and | 
find : 


') TisspRAND, Traité de Mécanique Céleste I p. 171. 


, di : ete AG) ’ . : 
*) For Mercury I get: — =+0%.573; sini —-? — — (049; SEELIGER gives: 


li 1°), 
+ 0.574 and — 0.049. For Venus I get: - = + 0".163; sin is. = + 0”.091; 
¢ 


at 


SEELIGER: + 07.159 and + 0.088; the small difference is owing to the value I 
get for C; = 2.286, while from SsELIGER’s data follows Cy = 2.217. 


28 


OV 2) C. ain J au 0.5986-8 OS 
= — 53 3 ge 20 (—Ca O 8 108 — = od 5 y— ; 
) mrga7e (a°—e 4, Sued C 3 [0.5 | 3 
where the number within brackets is a logarithm. 
Further: 
0d ; 0d 
——— sn Bb; —=—cosD®; ©=—40°1'8; 
Op 0g 
therefore 
OJ 0d 
F~ = =- [0/8083 —1]; === — [0.88414] 
Op 0g 
therefore 
oR : OR ; 
~—= 4 [0.4069—8]; — = + [0.48278]; 
Op 0q 
from which follows, taking as unit of time the century : 
Uy I 
P — + 9".065; — = — 0".054. 
dt dt 


Perturbations caused by the second eltipsord. 


Here the caleulation is much simpler. Introducing : 
ie) ioe) 


Ek du r= > du EB =f. du 

i =| (@+tu)Vcit u + =| (a? + u)? Vetu oJ (8 +a)? (2+ wu)" 
0 0 0 

we find: 


i 3 Ike 5 
S2 = H,—a,*B, — 4, be — (a?—c?) a,°E, sin | Fide cos2yp 


As a verification I have here also computed the perturbations of 
the inclination and longitude of the node for some of the other 
planets *). 

To compute the perturbation of the obliquity of the ecliptic I take: 


sin? J 
V = — Faga’e (a? —c’) E,a,? oi 
According to Srenieer’s data a= 1.2235 and c= 0.2399; I get 
di slat a REO : 
1) For Mereury I find: 7 = A060 sie a = — 0”.013; SEELIGER gives: 
€ f 


s di d 
— 0.057 and — 0.016. For Venus I find: = -+ 0’.007; sinz =>) sills) 
d ¢ 


SEELIGER: + 0”.009 and + 0”.144; the results differ somewhat; however, cal- 


dS 
culating according to SEELIGER’s formulae, for Venus I find: siz 2 = -+ 0”. 154. 


29 


B, = 2.445, log g = 0.8582—9 ; 


OV oJ e 
= [0.3401—7] ae @ = 74°22! (1900.0), J = 7°15’; 
therefore 
OS A OS 
— — [0.98361]; — = — [0.48051]; 
Op 0g 
therefore 
V ry QoQ co] OV Ne » 
a = + [0.3237 —7]; ag = + [0.7706—8] ; 
from which, taking as unit of time the century, | get: 
dp A dq , 
— == + 0".125; — = — 0".447. 
ay t at 


Therefore the perturbation caused by both ellipsoids together is: 


dp " dq 
— = + 0".190; — = — 0".501. 
dt dt 

Let « be the obliquity of the ecliptic for the time ¢, ¢, the same 


for the time ¢,, ¢ and Q inclination and longitude of the node of 


the ecliptic for ¢ with reference to the ecliptic for ¢,, then: 
cos & = cos i cos &, — sini sin &, cos Sb, 
from which, differentiating, we get: 
de Cs ib We red ih) 
— sme dt = — smicosé, ae sin &, a (sin 2 cos S%) 
therefore for t= t,: 
de dq 
Gendt 
The perturbation of the obliquity of the ecliptic thus is = = — 0".507- 
cd 


The difference between observation and theory given by Nprwcoms 
is —0".22 + 0.18 (probable error); this thus becomes + 0".28. The 
addition to the planetary precession a is given by: 


da 1 dp a 
=— — = + 0".478. 


H. Perturbations of the motion of the moon. 


We shall now proceed to the formulae for the computation of 
the perturbation of the motion of the moon. As the perturbative 
foree in the motion of the moon we have to take the difference 
between the attractions of the ellipsoid on the moon and on the 
earth. Suppose a system of coordinates, the sun at the origin, the 
axis of z perpendicular to the eliptic; let a, y,2 be the coordinates 


30 


of the earth in this system, 7+ § y+, 2+ those of the moon, 
then the projections of the perturbative force on the three axes 


are given by the expressions: 


OV OV OV OV OV ove 
& ir, idee © er dy | & ee Oz 


The ratio of the distances sun-earth and earth-moon being very 
large, IL develop in powers of §, 7,6, neglecting second and higher 
powers. Then the expressions for the perturbative forees are: 

OV VE Ve Oy eV OV 02V, eV a ¥. 
Oa? SD dd cps Oxdz = dxdy if dy” tints oon dxdz a dy0z ts Oz? 
and one can introduce as the perturbative function the funetion 


parler et a ee 
eae ons eel oe a ea loss ak fen age , 


Sr 


sn 


det | bady |? dade 

Here for v2, y,2 are to be substituted their expressions in elliptic 
elements and then the secular portion of F is to be taken. Since 
the powers and products of §, 4,6, contain only the elements of the 
orbit of the moon, the coefficients on the contrary only the elements 
of the orbit of the earth we can take the secular portion of each 
separately and multiply these together. 

Besides the system just mentioned suppose another system a’, y/’, 2’, 
the sun also being at the origin, but the axis of 2’ perpendicular to 
the equatorial plane of the ellipsoid. Then we have 

z =asin Psind, — y cos PsinJ, + zcosJ,, 
therefore 
de! 02! dz! 
a = sin P sin J,; a = — cos sind; a COS eee 
Perturbations caused by the jirst ellipsoid 
V 
From the expression given for £2———-— we deduce, negleet- 
aga 
ing the terms having sin? J as a factor: 


0 :. ~ du 42” 
Oia ay | (@tu(etuh | (apap bay 


72 4uy 


dady (a? 2) (+A) 


oO 
072 4u2' ot Ue geet! : du 
— (a°—c’?)— 2 (a?—c’?) sin D sin J, | - 


dede  (@ Lay a) | pw? (puis 


31 


72 ae 2 du |! Ay? 
Oy? i 4 (a? +-u)? (c?+u)le — (a?+2)? (ce? +4)'b 


os) 


072 Aye! ° 
= = (a7 —c¢7) + 2i(a? cos P re 
OyOz (a? A)? (c? +-a)*2 te Jase oN coe rie Se uy? u)? (c?-Lu)t2 


Q 


du du 
<1 A OE ea ee) Oe 
(a? tu)? (c2 + up'e AC +u)? (c? + u)'h 


Substituting the elements of the oibit of the earth for a, y, 2 and 
neglecting the second and higher power of the excentricity I get: 


72 2 C72 072 
=— ere N) 2 
0a? Ly °p Oy dady 
0°2 = 2(a*—c?) : 
a a J, — 2 (a’—c’) C, sin B sin J, 
Owdz a, Pp 
072 2'a? —¢?) ; : J 
aa _=— Tape cos D sin J, + 2(a?—c?) C,cos B sin J, 
inte 1 
072 


—_ == — 20, — 2(a?—c’) Cy. 


Let o be the radius vector, v the true anomaly, © the longitude 
of the perigee, §% the longitude of the node, 2 the inclination of the 
orbit of the moon, then we have : 

§ = 0 [cos (v + © — §{Q) cos §}, — sin (v +0 — Sp) sin S% cost] 
4 =0 [cos (v+- O—§h) sin [ + sin(v+O — Sb) cos Hh cos 7] 
$= osin(v+@—Jy) sini. 

1 write these expressions thus: 


= 0 (A cos v + Basin v) 


gn 


y= 0 (Cocos v + Dsinv) 
= 0 (Leos v + F sin v), 


Vas 


A, B,C, D, FE, F being expressions not containing the true anomaly. 
For the formation of the required products we need the secular 
portion of 0° cos? v and 9? sin’? v; I get: 
So? cos? v=a',* (4 + 2e?) Sg? sin? v= ka’? (1—e’) 
a, being the semi-major axis of the lunar orbif. 
Thus we get expressions as : 


eee (ae 


32 


* 92 v a . v 
Neglecting terms hke ¢* svn* >, e* sin‘ we get: 


2 2 
— —— — —— sin® (1—cos2 {X) + e? + — cos 20 
a, 2 4 4 4 
i 
3) le Fo me Sh io < 
— = — sin® isin2. 4+ — e? sin 20d 
es 4 
a, 
EO ee rey, 
= — sure sin \% 4- e@ su s 20)— \/ )— — sin 
73 5 sini sin 9) 1. ¢ hee in (2 \)) 9 oy 
Cf 1 =_ ~ = 
ve l i eC 2A) ee 3 5 ne 
— — —— sm" i(1 4+ cos2't) +e —— cos 2M 
Ge. 2 4 4 4 
75 ye ie hy 5 £ 3 , 
~~ — = sini cos () e* sin ————=COs(2@— a) cos Q, 
1g 5 9 5 ‘ 9 
ay, “ 2 a a a 
G le 
— == — sin* 4 
a Te 2 


Substituting in FR these expressions we get : 


Kagqate 1 a," 2 1 ey eel 
ees — “A -2C,a,?+—+ de? —C,a,* )+4sin" -—-C,(a°-c*)a,? 
R Cais zi P p 2 p 


: : 1 
+ 2(a?-—c?) sin J sin 2 cos ({i— ®) (2¢,— 4 j 
Pp 


The only perturbations to be considered are those of the longitude 
of the perigee and of the node. 
The differential equations required are : 
Ia 1 OR - dsl, 1 OR 


e— = - - sin 1 — == ——_ —. 


dt na,” Oe dt na," 07 


One easily perceives that the last term in the expression for 
gives no sensible perturbation on account of the factor a*—c’, the 


as 6 : ‘ : 
value of whieh is about Te. and of the facet that $2 has a period 
( 
of 18'/, years so that the coefficient we get by integration is about 
thirty times as small as would have been the case if {f had been 
absent. In the same way | omit the term (C,(a@’—c’*)a?, in the coeffi- 


cient of s7m>— and thus we have the following expression for FR: 


: <3 i f : 
I get C, = 0.678 ; — = 1.080 from which follows taking as unit 
PR 
of time the century : 


30 


Se arog: ©) ae Roh 33, 
dt dt 
- Perturbations caused by the second ellipsoid. 
I find: 
e2 d2 72 
SSS SS SS SS I = 
Ox? Oy? a dwdy 
2 Rpt ee : 072 Pay s 
—— == — 2 (a?—c’) E, sin B® sin J; ——— == 2(a? —c’) E, cos ® sinJ ; 
Oude ; Oy0z 5 
072 
== 2E, 2(a*—« a) Wee 


from which follows: 
R 1 a," 


k@mgase | 2.0," 


| == 2H ,a,” 


3h ,a,*e? — EB, (a®*—c?*)a,* sin? 2 


+ 2(a?—c¢?) a,” E,,sin J sin t cos (\i — ?)|. 
Although the term @*—c* is not small, yet it is. allowed to omit 
the periodic term. 
I get H, = 0.684, LH, = 2.445 from which follows taking as unit 
of time the century : 


do ; di. is 
SSS (IMEI 9 SS (J 
dt dt 

Thus both ellipsoids together give : 
UE iio oe. 
dt dt 


both insensible amounts. 


Astronomy. — “Remarks on Myr. Wourier’s paper concerning 
Seenieer’s hypothesis.” By Prof. W. pe Srrrer. 


(Communicated in the meeting of April 24, 1914). 


SeeLiger’s explanation of Newcoms’s anomalies in the secular 
motions of the four inner planets consists of three parts, viz : 

a. The attraction of an ellipsoid entirely within the orbit of Mercury 
The light reflected by this ellipsoid is, on account of the neighbour- 
hood of the sun, invisible to us. 

6. The attraction of an ellipsoid which inecloses the earth’s orbit. 
The light reflected by this ellipsoid appears to us as the zodiacal light. 

c. A rotation of the empirical system of co-ordinates with reference 

v0 


Proceedings Royal Acad. Amsterdam. Vol. XVI 


34 


to the “Inertialsystem’’. This rotation is equivalent with a correction 
io the constant of precession. The value of this constant which is 
implied in Newcoms’s anomalies is that used in his first fundamental 
catalogue (Astr. Papers Vol I). In “The Observatory” for July 1913 
I have shown that this constant requires a correction of + 1.24 
(per century). Consequently, of SretiGer’s rotation 7 only the part 
r, =r—1".24 ean be considered as a real rotation. 

The position of the equatorial plane of the ellipsoid @ was deter- 
mined by Serricer from the equations of condition: he found it not 
much different from the sun's equator. For the ellipsoid 6 the sun’s 
equator was adopted as the equatorial plane. 

It is important to consider the part which is contributed by each 
of the three hypotheses towards the explanation of the anomalies: 
By the way in which Sernicer has published his results this is very 
easy. It then appears that the ellipsoid a is practically only necessary 
for the explanation of the anomaly in the motion of the perihelion 
of Mercury, and has very little influence on the other elements. 
Similarly the ellipsoid 6 affects almost exclusively the node of Venus. 
The rotation 7 of course has the same effect on all perihelia and 
nodes. In the following Table are given Newcoms’s anomalies together 
with the residuals which are left unexplained by Segicer’s hypothesis. 
In addition to Seriicer’s residuals I also give residuals which are 
derived: A. by rejecting the rotation 7,'), and C. by omitting the 
second ellipsoid. The constants implied in the three sets of residuals 
are thus 
SEELIGER g,=2.18 X10 ¢,=0:31 K 105% 77a ee 

A 2.42 0.93 0 
C 2.03 0 + 6.85, 
where g, and g, are the densities of the two ellipsoids expressed 
in the sun’s density as unit. 
di 

Seeiicer did not compute the value of rr for the earth. The resi- 
dual given in the table is derived from the preceding paper by 
Mr. Wor Tder. 

From the table it appears that the residuals C are quite as satis- 
factory as those of Srxiicer. Consequently the ellipsoid 6 is not a 


1) The residuals A have already been given im the above quoted paper in “The 
Observatory”. The density g, is there erroneously given as 0.37 instead of 0.93 
(the correction to Seeticer’s value having been taken-as 0.2 limes this value, 
instead of 2.0). | have used the figures as published by SeeLiger. The small 
deviations found by Mr. WoLtsER are of no importance. 


: bys) 


necessary part of the explanation. Of the residuals A on the other 
hand there are, amongst the 10 quantities which were considered 


Mercury Venus | Earth | Mars 
de 
Fi NeEwcome | —0”.88 +0”.50 | --0/.21 +0”.31 | -++0/”.02 +0”.10 | +-0’.29 +0”.27 | 
| | | 
Newcoms | +8 .48 +0 .43| —0 .05 +0 .25/-+0 .10 +0 13) +0 .75 +0 35 
dw Ci, —0 .01 | —0 10 | +0 .03 | +0 .16 
“dt [/ 0 .00 0 .05 |+0 .18 0 52 
Cc -—0 .02 |—o 12 —0 .04 | 0 .00 
Newcoms |-++0 .61 +0 .52;+0 .60+0 17). ..... | 40 .03 +0 .22 
|—o 04 +0 .02 ona Men area |—o .20 
sin paels 
+0 .55 +0 .01 —0 .11 
—O0 31 +0 .05 —0O .24 | 
NEWCOMB | +0 .38 +0 .80 | +0 .38 +0 33)—0O .22 +0 .27 | —0 .O1 +40 .20)| 
a (seni |—0 .14 ‘| +40 .21 (40 .28) |+40 .01 
dt )4 =) 2 | +0 aN al He) +0 .05 
& —0O .15 +0 .23 —0 17 —0 .01 


by Srrnicger, 3 residuals exceeding their mean error. This in itself 
would not be sufficient to condemn the hypothesis, but the residual 
for the secular variation of the inclination of the ecliptic (+ 1'.18) 
is entirely inadmissible. We conclude therefore that the rotation 7, 
is a vital part of the explanation. 

The great influence of the ellipsoid 4 on the ecliptic is, of course, 
due to the large inclination of its equator. If this equator was e.g. 
supposed to coincide with the invariable plane of the solar system, 
instead of with the sun’s equator, this influence would be much 
smaller. It is impossible to decide a priori whether it will be found 
possible so to adjust the position of the equator and the density of 
this ellipsoid that it has the desired effect on the node of Venus 
without appreciably affecting the earth’s orbit. 

The motion of the node of the earth’s orbit is the planetary pre- 
cession. Calling this 4, we have, for t= t, 

3* 


36 
ne dp 
=a 


where p is the quantity so called by Mr. Wortser. We thus find 
for the three hypotheses 


Ad. sine 


SEELIGER Ah = + 0".47 
A +1 13 
Cc +0 15 


Newcoms did not include a deviation between observation and 
theory for this quantity. At the time of the publication of the 
“Astronomical Constants” (1895) it was of course entirely correct 
to consider a determination of the planetary precession from obser- 
vations as impossible. Since that time however very accurate invest-' 
igations of the precession have been executed by Nrwcoms himself 
(Astr. Papers, Vol. VIII) and by Boss (Astr. Journal, Vol. XVI, 
Nrs. 612 and 614). Now the precession in right-ascension depends 
on the planetary precession, but that in declination does not. We 
have 

m = lcos €—) 
n=lsine 
/ being the lunisolar precession. 

Newcoms determined / from the right-ascensions and the declina- 
tions separately, and found a large difference in the results. If this 
were interpreted as a correction to the planetary precession, we 
should find 

A= 0747. 

Boss determined m and 2 separately, the latter both from right- 
ascensions and from declinations. From his results I find (applying 
the correction of the equinox Ae — + 0.30, adopted by both Boss and 
NEWCOMB) : 


Ah = + 0".85 + 0".22 
The mean error does not contain the uncertainty of the correction 
Ae. Its true value probably is about = -+ 0".25. The mean error 


of the value of 42 derived from Nrwcome’s work is difficult to 
estimate; we may assume it to be equal to that of Boss. The mean 
of the two determinations would then be 
Aa = + 0".66 + 0".181). 
1) Also L. Srruve (A. N. Vol. 159, page 383) finds a difference in the same 
sense. Neglecting the systematic correction », | find from his results 
Ar = + 0".93 + 0".80. 
The m. e. again is too small as it does not contain the effect of the uncertainty 
of the correction ». 


o7 

Now it is certainly very remarkable that this correction is of the 
same sign and the same order of magnitude as the planetary preces- 
sion derived from the attraction of Srenicmr’s ellipsoids. It must however 
be kept in mind that it is very weil possible to explain the disere- 
paney between the determinations of the constant of precession from 
right-ascensions and from declinations (or from m and from 7) by 
the hypothesis of systematic proper motions of the stars. Thus Hoven 
and Haum (M. N. Vol. LXX page 586) have from the hypothesis of 
unequal distribution of the stars over the two streams derived a 
systematic difference which is equivalent (for Newcoms) ‘) to a correction 

Ai = + 07.56. 

As the effect of the attraction of SepricEr’s ellipsoids on the motion 
of the moon Mr. Wortser finds a secular motion of both the perigee 
and the node. Both of these are due chiefly to the inner ellipsoid 
and are thus not much altered if Seeticur’s hypothesis is replaced 
by either of the hypotheses A or C. We find 


dw ASG et 

SRELIGER a SL OTL SS = HN) 
dt dt 

A 4+. 2.04 135.30 

C + 2 10 —-2 .06 


All these quantities are well within the limits of uncertainty of 
the observed values. 


Chemistry. — “Vhe application of the theory of allotropy to electro- 
motive equilibria.” Ul. By Dr. A. Smits and Dr. A. H. W. ATEN. 
(A preliminary communication). (Communicated by Prof. J. D. 
VAN DER WAALS). 


(Communicated in the meeting of April 24, 1914). 


1. In the first communication *) under the above title it has been 
demonstrated that the theory of allotropy applied to the electromotive 
equilibrium between metal and electrolyte, teaches that a metal that 
exhibits the phenomenon of allotropy and is therefore built up of 
different kinds of molecules immersed in an electrolyte, will emit 
different kind of ions. 

The different kinds of ions assumed by the theory of allotropy, 
need not be per se different in size, as was remarked before. They 


1, For Struvn’s stars the correction would be + 0”.77. For Boss the corre- 
sponding computation has of course not been executed by HouaH and Hats. 
*) These Proc. Dec. 27, 1913, XVI. p. 699. 


38 


may be equal in size, but different in structure. There can, however, 
be another difference besides, viz. in electrical charge. In the preced- 
ing communication the molecule kinds J/ and J/, were assumed, 
and for simplicity’s sake the circumstance that part of these molecules 
are electrically charged also in the metal, was not mentioned. This 
circumstance need not be taken into account, because the electrical 
charge of the atom J/ in one ion JJ/,*) was put equal to that in 
the other ion (J2-*). If it had then been our intention to indicate 
the total equilibrium in the metal, we might have drawn up the 
following scheme : 


2M@M°+602M=+60 (1) 
QV eo 
2M Fe M, (4) 
from which follows that the system would then be pseudoquaternary. 

For an explanation of the electromotive disturbances of the equi- 
librium mentioned in the preceding communication, a consideration 
of the equilibrium (1) or (4) sufficed. Then equation (4) was chosen 
and 2M and M, were therefore called the pseudo components, 
though of course we might as well have taken 2M: + 66 and 
MM. + 60. 

Now it is clear that when in the metal ions of equal structure 
occur, but of different value, the scheme of equilibrium can be as 
follows. 

M-+202M-:-+30 (1) 
(2) XS [ Ly (3) . i 


The system is then pseudo ternary, but in most of the cases it 
will be sufficient to consider the pseudo binary system, indicated by 
equation (1), and assame MW: +20 and M--+30 as pseudo 
components. A similar equilibrium will have to be assumed, when 
the metal can go in solution with different valency under different 
circumstances. This case is probably of frequent occurrence. 

Of course the metal phase is already complex, when metal ions 
occur by the side of uncharged molecules, but this complexity does 
not suffice to explain the peculiar electromotive bebaviour of the 
metals, whereas schemes I and II are competent to do so. 

In connection with the foregoing considerations it could be shown 
that the unary electromotive equilibrium finds its proper place in 
the 4,2 figure of a pseudo system, which ean clearly appear under 
certain circumstances, when we namely sueceed in bringing the 
metal out of the state of internal equilibrium. Thus it was e.g. shown 


that when a metal is brought to solution by an electrolytic way, so 
when it is made into an anode, the internal equilibrium will be 
disturbed, and the metal will become superficially enobled, at least 
when the velocity of solution is greater than the velocity with which 
the internal equilibrium sets in. In this case therefore the dissolving 
metal will have to become positive with respect to an auxiliary 
electrode of the same metal which is superficially in internal equi- 
librium. If reversely the metal is made to deposit electrolytically, 
the reverse will take place, and the separating metal will be less 
noble and therefore negative with respect to the auxiliary electrode. 

The anodie disturbance of equilibrium being attended with a dimi- 
nution of the more active kinds of molecules, this process will bring 
about a diminution of the chemical activity. This is therefore the 
reason that this anodic state of disturbance is a more or less passive 
state of the metal. 

At the eathode the disturbance lies exactly in the other direction, 
and a more active state will be brought about. 

The degree in which a metal is thrown out of its state of equi- 
librium in case of electrolytic solution or deposition, will depend 
on the current density at constant temperature, and it was therefore 
of importance to study the discussed phenomenon at different current 
densities. 

What may be expected is this that the internal equilibrium will 
generally be able to maintain itself for very small current densities. 
Then the tension with respect to the auxiliary electrode will be 
zero, both when the metal is anode and cathode. With greater 
current densities the metal will get superficially more and more 
removed from the state of internal equilibrium on increase of the 
current density, and the tension with respect to the auxiliary elec- 
trodes will greatly increase. 

As the metal surface gets further removed from the state of 
internal equilibrium, so becomes more metastable, the velocity of 
reaction which tries to destroy the metastability, increases however 
in consequence of the change of concentration in the homogeneous 
phase; and we may therefore expect that the potential difference 
between metal and auxiliary electrode will vary with the current 
density in the way indicated in Fig. 1. 

When the velocity with which the internal equilibrium sets in, 
is small, the part a) will lie at exceedingly small current densities, 
and if the measurements are not exceedingly delicate, we shall get 
the impression that this piece is entirely wanting. 

lt is clear that the tension which is represented here as function 


40 


of the current density means the tension with respect to the auxiliary 
electrodes. This tension, which is also called polarisation tension, is 


Polarisation. 


Fig. 1. 


positive when the metal is anode, and negative, when it is used 
as cathode. 

Further this possibility was still to be foreseen that when the 
metal assumes internal equilibrium very slowly a distinct change of 
the potential difference would have to be demonstrated even after 
the current had been interrupted. 

Now it shonld be noted here that when a base metal has become 
noble during its use as anode, and the difference of potential between 
the metal and electrolyte has risen to the tension of liberation of 
the oxygen, at the anode two processes will begin to proceed side 
by side; besides the going in solution of the metal we get also the 
discharge of the OH’-ions and the possible formation of oxide skins, 
the influence of which should be examined. 

We get something of the same kind at the cathode. When viz. 
the difference of tension metal-electrolyte at the cathode has become 
ereater than the tension of liberation of the hydrogen, besides dis- 
charge of metal ions, also discharge of H’-ions will take place there. 


Method of Investigation. 
The measurement of the polarisation tensions took place in the 


following way (see Fig. 2). Two electrodes of the metal that is to 
be investigated, in the shape of wire or rods, were placed in a solution 


41 


of a salt of the metal, generally the nitrate. The two electrodes 
were connected by a variable resistance and an Amperemeter with 
a number of accumulators, so that the strength of the polarizing 
current is easily changed and measured. To measure the tension of 
polarisation at one of the electrodes a beakshaped bent glass tnbe 
was brought into the solution, whose capillary point was placed as 
close. as possible ‘against the polarized electrode. In this glass tube 
a third (auxiliary) electrode of the same metal was brought. This 
auxiliary electrode, which is currentless, exhibits the normal potential 
difference with respect to the solution. As there is no loss of tension 
in the liquid of the auxiliary electrode, and its point is close against 
the polarized electrode, the potential difference between the auxiliary 
electrode and the polarized 
electrode gives directly the 
deviation which the potential 
difference of the polarized 
electrode presents from the 
normal potential difference, 
so the polarisation tension. 


The measurement of this 
potential difference took place 
by reading the deviation 
which was obtained by con- 
necting the auxiliary electrode 
and the polarized electrode 


by means of a resistance of 

_ Fig. 2. some meg. ohms with a gal- 
vanometer. The value of the scalar divisions in Volts was determined 
by connecting the galvanometer with a normal element. 


Silver, Copper, Lead. 


2. The investigation of different metals, undertaken in this direc- 
tion, has shown us that as was to be expected, they represent the 
most different types. 

There are metals which in contact with an electrolyte, assume 
internal equilibrium very quickly ; there are those that do so very 
slowly, and there are those that lie between these extremes. 

Beginning with the metals which quickly assume internal equili- 
brium, we may first mention the metals: sé/ver, copper and lead. 

The result of the investigation of these metals is found in the 
following tables. 


4 


be 


After the current had been interrupted, no potential difference with 
the auxiliary electrode was to be perceived. 

In the first column the current density is found expressed in milli- 
amperes per em*®. In the second column the potential difference with 
the auxiliary electrode is indicated in Volts, the metal serving as 
anode (anodic polarisation tension); and in the third column the 
same is given for the case that the metal served as cathode (cathodic 
polarisation tension) 


/ 


AB Es 
Silver electrode immersed in 1/, N, Ag NO3-solution. 
l 

: = ne V-anode V-cathode 
25 + 0.03 — 0.006 
50 + 0.03 —— 0.012 
100 + 0.04 — 0.014 
200 + 0.05 — 0.015 
300 + 0.05 — 0.016 
400 + 0.06 — 0.018 
750 + 0.09 — 0.020 


It is seen from this table that the silver is not materially nobler 
during the solution, and not materially baser during the deposition 
than the auxiliary electrode, which is entirely in internal equilibrium. 
The polarisation is therefore exceedingly slight here, from which we 
may deduce that the metal silver very quickly assumes internal 
equilibrium. Under these circumstances it is of course out of the 

TABLE 2. 
Copper electrode in '/. N.Cu(NOs))-solution. 


| 
= = uae V-anode V-cathode 
14 + 0.016 — 0.016 

29 + 0.026 — 0.026 
57 | + 0.032 — 0.035 
114 + 0.048 — 0.063 
171 + 0.048 — 0.082 
930 + 0.050 — 0.088 


43 
question that a potential difference could sull be demonstrated after 
the current had been broken, which accordingly was by no means 
the case. 
For copper the following values were found. (See table 2 p. 42). 
This is, therefore, the same result as was obtained for silver, and 
lead behaves in an analogous way, as appears from the following table. 


TAB EES 3: 
Lead electrode in 1,.N.Pb(NO3)-solution. 


2 — ne V-anode | V-cathode 
36 + 0.010 — 0.006 

140 + 0.033 — 0.010 
280 -L 0.046 — 0.013 
510 | + 0.082 — 0.017 
1000 «=| «40.126 =| . — 0.020 


| 


After the current had been interrupted no potential difference with 
the auxiliary electrode could be demonstrated. 


Nick ‘el ° 


3. A splendid example for an internal equilibrium setting in very 
slowly is furnished by nickel, as appears from the following result. 


TABLE 4. 
Nickel electrode immersed in '/, N . Ni (NO3),-solution. 
5 | V-anode V-cathode 
| ——. 
21— | +1.61 — 0.95 
ra Nigel hg 
Cine 4 SET GES ES ho 
180 + | + 1.77 — 1.40 
360 | +4 1.83 | 1166 
540 | STEER |b eles yg 


Nickel shows therefore an enormous anodic and cathodic polarisa- 
tion, which we must ascribe to the very slow setting in of the 
internal equilibrium, the more so, as we found that even after the 


44 


current had been interrupted a great potential difference with the auxili- 
ary electrode could still be demonstrated viz. an anodic polarisation 
tension of 0,95 Volt. and a cathodic polarisation tension of 0,5 Volt. 
These tensions decreased with diminishing velocity to 0, as a proof 
that the metal assumes internal equilibrium by the aid of the 
electrolyte. As on account of the osvillations of the mirror of the 
galvanometer the said tensions could not be observed quickly enough 
after the current had been interrupted, the above values give the tensions 
some seconds after the interruption of the current. Immediately after 
the interruption they willhave been + 1,88 V resp. — 1,77 V. Hence 
nickel, used as anode, becomes superficially a metal nobler than 
platinum as we know it. 


Cadmium. 


4. Cadmium is a metal lying between silver, copper, and lead 
on one side and nickel on the other side with regard to the velocity 
with which its internal equilibrium sets in. 

For this metal we found what follows; 


TABLE 65. 


Cadmium electrode in !/> N. Cd (NO3)o-solution. 


d | V-anode V-cathode 
21 |) 220h093) | —n027 
et Stats | — 0.186 
144 | + 0.290 | — 0.220 
286 | + 0.380 | = 0.220 
428 | + 0.507 | — 0.220 


Besides that the polarisation is smaller here than for nickel, it is 
noteworthy that while for nickel the anodic and cathodic polarisa- 
tion tension differ little, this difference becomes pretty considerable 
for cadmium, at least for large current densities. This peculiarity 
may be explained in a simple way by means of the A,z-figure given 
in the preceding communication. (See Fig. 3.") 

Suppose that with unary electromotive equilibrium at the given 
temperature the electrolyte 4 and the metal phase S coexist, then the 


1) Here the potential difference of the metal with respect to the electrolyte has 
been given. 


45 


metal phase in case of anodic polarisation will move from S to 6, 
dA 


and over this range — is great. 
Ae 


In case of cathodic polarisation the metal phase moves from S§ 
upwards along the line SC, but here we see now that the quantity 
END ee : : 
= will continually decrease and can become very small in consequence 
of the ever increasing curvature of the line SC, which can be even 
a great deal more pronounced than has been drawn here. 

It now follows from the observations that the metal cadmium 
assumes internal equilibrium pretty rapidly, and in harmony with 
this is the fact that after the current had been broken the polarisa- 
tion had soon entirely vanished. 

It was besides noticed in this investigation that the metal which 


46 


Served as anode, was gradually covered with a skin of basic salt. 
It was, however, easy to demonstrate that this skin could not have 
caused the observed phenomena through increase of the resistance, 
for the phenomena remained the same also when this skin, which 
could be very easily removed, was taken away during the electro- 
lysis. Moreover it appeared that when this metal with skin was 
made to cathode, the cathodic polarisation was the same as in the 
absence of this skin. The formation of the skin is therefore a secon- 
dary phenomenon, as was also expected (see under 1). 


bismuth. 


5. bismuth is a metal that very clearly seems to be catalytically 
influenced, as appears from the following table. 


TABLE 6. 
Bismuth in '/9 N Bi(NO,)-solution. 


5 | V-anode | V-cathode 
35 AE S02 a = 0802 
G0) ie OROL en OF08 
133 © |) St eDs050 le =aulov03 
2600) | Zeal S14el =. 50803 


The anodie polarisation presents this particularity that though it 
is exceedingly small up to a current density of 133 milli Amperes 
per cem*, as for silver, it becomes pretty considerable for a current 
density of 260 milli Ampeéres. Now it is worthy of note that the 
anodic polarisation was at first also small for a current density of 
260, but if increased slowly, so that it amounted to + 1.14 volts 
after a few minutes. For smaller current densities, however, no rise 
of the polarisation tension took place in course of time. The explanation 
of the observed phenomenon is probably as follows. The Bismuth, 
which gets positively charged in the used solution, assumes internal 
equilibrium very quickly at first. At the greatest density of current, 
however, this internal equilibrium is no longer able to maintain itself, 
and then generation of oxygen seems to take place, which oxygen 
evidently exercises a negative, catalytic influence, which renders the 
metal still nobler. This phenomenon being attended with the formation 


Al 


of a white skin (probably of basie salt) we have again examined 
what influence this skin exercises on the phenomenon. For this pur- 
pose the current was suddenly reversed, after a thick layer of the 
basie salt had formed, in which however, only a cathodic polarisation 
of 0,18 Volt was observed as a proof that this skin, indeed, increased 
the resistance somewhat, as was expected, but that this could have 
been only of slight influence on the amount of the anodic polarisation 
tension’). What the negative catalytic influence here consists in, 
cannot be said with certainty, but as has been stated, it seems 
probable to us that the oxygen, dissolved in the metal to an exceed- 
ingly slight degree, retards the setting in of the internal equilibrium. 


Tron. 


6. If we now proceed to the metal iron we meet again with 
phenomena, and very pronounced ones too, which in our opinion 
point to catalytic influences. 

We found the following result : 


TABLE i: 


Iron electrode immersed in !/) N.FeSO,-solution. 


0 | V-anode 

50 0.026 
100 | 0.038 
130 0.044 
160 | 0.064 
199 0.075 
250 | 0.113 
300 | 0.164 
400 2.25 
600 2.47 
800 2.53 


from which it appears that in this transition of a current density 
from 300 to 400 the iron has suddenly become very noble. This 


1) For it ean hardly be assumed here that the skin offers a different resistance to 
currents of different direction. 


4s 


phenomenon, whieh has been already often observed, and is called 
the becoming passive of iron, has not been accounted for in a 
satisfactory way. 

In the light of these new considerations the explanation, as was 
already observed, is not difficult.) The iron, which shows. this 
sudden increase of the anodic polarisation, is entirely free from so- 
called annealing colours and_ perfectly reflecting, so that an oxide 
skin is out of the question. 

If we, however, assume that the metal dissolves a little oxygen, 
and this oxygen retards in a high degree the setting in of the 
internal equilibrium, the sudden considerable enobling of the metal 
is explained in a simple way. 

Up to now it has been lost sight of too much that the pheno- 
menon of passivity, arisen by an electrolytic way, and that called 
into existence by a purely chemical way, must be explained from 
one and the same point of view. By a purely chemical way iron 
is made passive by being simply immersed in strong nitric acid for 
a few moments. If then the iron is put in a solution of copper 
sulphate, the copper does not deposit. By a shght shake, the appli- 
cation of a magnetic field ete. this passive state can, however, 
at once be destroyed, and the iron is covered with a coat of 
copper. 

If we consider the passive iron to be iron that is superficially 
very far from the state of internal equilibrium, in which super- 
ficially the easily reacting molecules are practically entirely wanting, 
and assume that this state can be maintained for some time on 
account of the negative catalytic action of oxygen under certain 
circumstances, which state, however, outside the cell, can be destroyed 
by vibrations, a magnetic field ete., the phenomenon of passivity 
of iron becomes less unintelligible. *) 

Returning to the experiment, we will show in the first place 
what was found when smaller current densities were worked with 
after the iron had become “passive” at higher current density. 

This table exhibits therefore the great difference between the passive 
and the active iron. As appears from the last table but one, the 
active iron yields a difference of tension with the auxiliary. electrode 
of 0,026 Volts for a density of current of 50; the passive iron yields 
a difference of tension of 2,18 Volts for the same current density. 

i) Suits, These Proc January 25, 1913, XVI. p. 191. 


2) We have probably to do here with metal ions of different valency. (We shall 
return to this later on.) 


49 
; TABLE 8. 


iron electrode, immersed in ''5 NFeSQO,-solution. 


‘ V-anode | V-cathode 
800 DOS 0 50 
600 2.47 | 0.47 
400 2.40 0.44 
200 | 2.30 | 0.42 
100 2.24 | 0.37 

50 | 2.18 0.27 


It is now remarkable that, as has also been found by others, 
contact with hydrogen can annihilate the passivity. When we reversed 
the current and made the passive anode the cathode for a moment, 
and then reversed the current again at a density of 400 m.A., the 
difference of tension with the auxiliary electrode amounted at first 
only to 0,12 Volt, but this tension rose at first rather slowly to 
0,6 Volt and then rapidly to 2,27 Volts. 

It therefore appears from this experiment that hydrogen is a 
positive catalyst for the setting in of the internal equilibrium of 
iron. which also accounts for the fact that the cathodic polarisation, 
as appears from the last table, is extremely small in comparison 
with the anodic polarisation. The difference between anodic and 
cathodic polarisation is therefore so great here, because for the 
anodic polarisation a negative catalyst, and for the cathodic polarisa- 
tion a positive catalyst come into play. 

That for nickel the anodic and the cathodic polarisation are about 
the same proves that the oxygen and the hydrogen do not act 
noticeably catalytically on this metal. 

It should finally still be pointed out that when at the moment 
that the passive iron had veached an anodi¢ tension of polarisation 
of 2.27 Volts, the current was broken, still a tension of polarisation 
was observed of 1,07 Volts, which tension, however, pretty quickly 
fell to O. So it appeared just as for nickel that the iron without 
passage of the current soon assumes internal equilibrium by the aid 
of the electrolyte, and becomes active. We see from this that the 
hegative catalytic action is maintained by the current; when the 
current is broken the active iron above the liquid will, however, 

4 

Proceedings Royal Acad. Amsterdam. Vol. XVII. 


50 


promote the setting in of the internal equilibrium in the at first 
passive part, and this will be the explanation of the fact that the 
iron becomes active after the current has been broken. 

Also after the use of the iron electrodes as cathode the current 
was broken, and as was to be expected, the much smaller cathodic 
polarisation tension of + 0,15 appeared to run very rapidly back to 0. 


Aluminium. 


7. As far as ifs electromotive behaviour is concerned, aluminium 
is undoubtedly one of the most interesting metals. For anodie pola- 
risation the current density decreased regularly, and the tension 


increased, as is shown in the following table. 


TAB EE V9: 


Aluminium electrode in !y NAlo (SO4)3-solution., 


; L 
0 V-anode 
0.8 + 2.56 
0,53 Ly 
0,46 | + 3.84 
0,36 = | ate ASD 


Accordingly we find anodie polarisation tensions of about 4 Volts 
for this metal already at very small current densities, which points 
to the fact that here a layer of great resistance must have been formed. 

Up to now it has been tried to explain this strong anodic polari- 
sation for aluminium by the formation of an insulating skin of Al,O,. 
With greater densities of current the anode is really covered with 
an oxide skin, and it is therefore natural to assume the formation 
of this skin also for smaller densities of current, and attribute the 
observed phenomenon to this skin of Al,O, with great resistance. 
There are however objections to adopting this explanation, for in 
our experiments no trace of annealing colours was to be observed, 
and the metal remained beautifully reflecting. 

To ascertain whether in our experiments a skin of great resistance 
had formed round the anode, we made the following experiment. 

The bottom of the vessel with the Al?(SO,), solution was covered 
with a layer of mercury, and the aluminium electrode was anodi- 


51 


éally polarized. When this electrode was now covered with a skin 
of great resistance, an immersion of one extremity of the aluminium 
electrode in the mereury should not exert any influence on the 
difference of tension between the aluminium anode and the auxiliary 
electrode. If, however, this skin does not exist, the aluminium elec- 
trode will get into contact with the mercury during the just described 
manipulation, and the said difference of tension will be modified. 

The result was that when during the anodic polarisation the 
aluminium anode was immersed in the mercury, and the current 
was then broken, the difference of tension with the auxiliary elec- 
trode was absolutely unchanged, which proved therefore that the 
aluminium electrode did not get in contact with the mercury, but 
was surrounded with a coat of electrolyte. This appeared to be no 
specifie property of the anode, for the same thing was observed after 
cathodic’ polarisation. An unpolarized Al-wice, immersed from the 
electrolyte in the mercury layer, immediately assumed the potential 
of the mercury, from which therefore follows that the gas layer on 
the aluminium retains the electrolyte with great force. 

In this way the question of the skin could therefore not he solved. 
What is remarkable is this that the skin formed during anodic 
polarisation, immediately seems to disappear again by cathodic 
polarisation. The assumption of a film of Al,Q, is attended with 
great difficulties, in the first place this oxide cannot be reduced 
under these circumstances by H in status nascens, and in the second 
place it appears, that nothing is to be perceived of this skin, at 
least with the naked eye, as no annealing colours are to be observed, 
and the metal remains clearly reflecting. It seems therefore not too 
hazardous to us to conclude in virtue of this that the skin cannot 
be an oxide layer, and the only thing left to us is to assume, as 
we did for iron, that the oxygen dissolves in the aluminium during 
anodie polarisation, and that this solution possesses a great electric 
resistance for aluminium. In this way we come to the assumption 
of a layer with great resistance, of which it is, however, to be 
understood, that it entirely disappears on cathodic polarisation to 
make room for a solution of hydrogen and aluminium. Accordingly 
this layer is metallic, and can amalgamate in course of time when 
in contact with mercury, through which the resistance disappears. 
The result at which we arrive is therefore this that the anodically 
measured tension is so extraordinarily great for aluminium, much 
greater than the liberation tension of O, can be here, because the 
dissolved oxygen not only retards the setting in of the internal 
equilibrium, but also a layer of great electric resistance is formed. 


52 


At greater current densities Al,O, can separate from this solution 
of oxygen in aluminium, but then the electrode is no longer reflect- 
ing, and it cannot be made reflecting again by cathodic polarisation. 
This layer of Al,O, can also possess a great resistance, but the 
primary feature of the phenomenon is in all cases the formation of a 
solution of oxygen in aluminium, which possesses a great resistance. 


If we now proceed to the description of the experiments with 
amalgamated aluminium, we will begin with stating that when in 
the just deseribed experiment the aluminium electrode was. raised 
ont of the mercury, after amalgamation had set in, and the lower 
opening of the auxiliary electrode was placed against the extremity 
of the aluminium wire, this part of the aluminium had undergone 
a great change, and had become negatively electrical with respect 
to the auxiliary electrode. The tension difference amounted to —0.9 
Volt, and still increased slowly. At the place where the aluminium 
had been in contact with the mercury, it had therefore become 
much baser, and had visibly become somewhat amalgamated. 

That amalgamated aluminium is baser than the non-amalgamated 
metal, was known, but the exact value of this difference in tension 
was not met with in the literature. To determine this difference in 
tension, an aluminium electrode was amalgamated by immersion in 
a solution of HgCl,, after which this electrode was compared with 
the auxiliary electrode. We found that the amalgamated Al obtained 
in this way was still baser than the just mentioned Al, for the 
tension of this electrode with respect to the auxiliary electrode 
amounted now to —1.27 Volts. 

That the amalgamation for aluminium has a very particular effect 
follows moreover from this that amalgamated aluminium possesses 
a much greater chemical reactive power than the ordinary alumi- 
nium. Amalgamated aluminium immersed in water gives a very 
considerable generation of hydrogen, and it oxidizes so rapidly when 
exposed to the air that the metal is immediately covered with a 
layer of oxide, the liberated heat raising the temperature of the metal 
very noticeably. 

In consideration of all this it seems more than probable to us 
that the action of mercury is here positively catalytic, and that mer- 
cury therefore, when dissolving in aluminium, brings the metal in 
internal equilibrium, which condition corresponds to a greater con- 
centration of the simpler, so more reactive kinds of molecules. 

The anodic polarisation of the amalgamated state is almost as 
slight as for silver, as a proof that the internal equilibrium sets in 


53 
much more quickly here than for pure Al, but not yet so rapidly 
as for Ag. 


Amalgamated Aluminium. 


Lo leaned V-cathode 

2 | + 0.03 

5) |) 420.07), |) = 0:05 

Ne a= ONS |= 0120 

33 | +018 | --033 i 
a7), 0.34 1 | 


That the amalgamated aluminium goes into solution much more 
rapidly than the non-amalgamated aluminium also appears from 
what follows. If a new aluminium electrode is put in the just men- 
tioned mercury layer, which covers the bottom of the vessel with 
the Al,(SO,),-solution, this electrode assumes the mercury potential. 
The tension difference with the auxiliary electrode is then namely 
+ 0,6 Volt, which tension difference is also found when a plati- 
num electrode is used instead of an aluminium electrode. If the same 
experiment is, however, made with an amalgamated Al-electrode, 
the tension difference with the auxiliary electrode is — 0,78 Volt. 
It follows from this that if the ordinary aluminium partially immer- 
sed in mercury, failed entirely to maintain its potential difference 
with respect to the electrolyte in consequence of too slow solution, 
the amalgamated aluminium does not quite succeed in this either, 


but it almost sueceeds, for instead of — 1,27 Volts its tension with 
respect to the auxiliary electrode has namely become — 0,78 Volt. 


lt is perhaps not superfluous to elucidate this phenomenon in a 
few words. With immersion of the aluminium electrode in the mer- 
cury a short circuited element aluminium-electrolyte-mercury is obtai- 
ned, in which the aluminium is the negative pole, and therefore 
sends ions into solution. If now the setting in of the internal equili- 
brium took place with great rapidity, the aluminium would be able 
to maintain its unary potential difference, and in this case the ten- 
sion of this electrode with respect to the auxiliary electrode would 
have remained — 1.27 Volts. Now we find —-0,78 Volt, proving 
that the state of internal equilibrium was disturbed to a certain 
extent after all, and the metal has become a little less base by 
dissolving. If, as was described, the same experiment is made with 


54 


ordinary aluminium, which is therefore an enobled state of aluminium, 
we get what fellows. 

The ordinary aluminium is at first the negative pole with respect 
to the mercury. It becomes, however, noble by the dissolving, and 
it is soon as noble as mercury. Nobler than mercury it can, howe- 
wer, not become then, since in this case, the current would be 
reversed, which would change the state of the aluminium again in 
the base direction. This is the reason that ordinary non-amalgamated 
aluminium immersed in mercury, assumes the potential of the mer- 
cury. This experiment can however not be continued for any length 
of time, because the aluminium in contact with mereury slowly 
amalgamates, as we have seen, in consequence of which finally also 
the part which is not in contact with the electrolyte, will become 
active, so that the same things will be observed as in case of well- 
amalgamated aluminium. 

In a following communication the investigation of the other metals 
will be treated, after which a critical summary will be given of the 
theories which have been proposed by others up to now as an ex- 
planation of some of the facts discussed here. 


SUMMARY. 


In the foregoing pages the theory of allotropy was applied to the 
electromotive behaviour of the metals Ag, Cu, Pb, Ni,Cd, Bi, Fe, Al. 

We have come to the conviction that the newly obtained point 
of view, as we hope to prove further, enables us to survey the 
widely divergent cases, and gives a deeper insight into the signifi- 
cance of the observed phenomena. 

Anorg. Chem. Lab. of the University. 
Amsterdam, April 23, 1914. 


Chemistry. — “The Allotropy of Cadmium.” Il. By Prof. 
Ernst Conen and W. D. HeELpEerMAN. 


(Communicated in the meeting of April 24, 1914). 


1. In our first paper on this subject') we concluded from measure- 
ments with the pyknometer and the dilatometer that cadmium has 
a transition temperature at 64°.9 and that this metal as we have 
known it until now, is a metastable system in consequence of the 
very strongly marked retardation which accompanies the reversible 


1!) These Proc. 16, 485 (1913). 


a) 


change of these allotropie modifications both below and above their 
transition points. As we pointed out in our papers on the allotropy 
of copper and zine, the possibility that there might be present at 
the same time more than two allotropie forms had to be taken 
into account. 

If this were the case, a variation in the previous thermal history 
might have an influence on the transition temperature. 

The samples which had given 64°.9 as their transition point 
(Vide § 11 of our first paper) only differed by the fact, that the 
second one had been in the dilatometer at 100° in contact with 
paraffin oil for 36 hours after having given 64°.9. At the end of 
this time the measurements were made, which are given in Table II. 
On continuing our investigations we got the impression that this 
difference in the thermal history of the samples might not have been 
large enough to determine whether a third modification can be 
formed. As a result of the following considerations we carried out 
some new experiments. 


2. If in our sample A, (first paper) there had been present 
originally more than two modifications, it might be possible that 
the greater part of the modification(s) which is (are) stable at higher 
temperatures had been changed into the ;“-form, as the sample 
had been heated at 101°C. for 24 hours in contact with a solution 
of cadmium sulphate. In this case the heating at 100°, which 
followed the first experiment with the dilatometer, might have had 
no perceptible influence on the transition point which is in accordance 
with the results given in tables I and II. 


3. We now varied the previous thermal history of A, very 
markedly. For this purpose the metal was taken out of the dilato- 
meter and chilled by throwing it into water. After this it was put 
into a new dilatometer without previously treating it with a solution 
of cadmium sulphate at 101°. The dilatometer was then kept at 
70°.0; the temperature remained constant within 0.003 degrees. The 
meniscus fe// in 3°’, hours 143 mm. while we observed formerly 
(first. paper) a strongly marked increase of volume at the same 


temperature. 

4. In order to control this result, we carried out the following 
experiment : 

A fresh quantity of the metal (‘‘KanLBaum’ — Berlin) weighing 


about 300 grams (A,) was melted and chilled. We then turned it 
into thin shavings on a lathe and put it into a dilatometer ; the bulb 


was filled up with paraffin oil and a quantity of small glass-beads. 
(Vide our first paper § 10). At no temperature between 50 and 100° 
(vide § 4 of our first paper) did any change occur. We then added 
100 grams of the same material A, which had been in contact with 
a solution of cadmium sulphate (at 50°) during 12 hours. We now 
observed that the meniscus of the dilatometer 


fell 167 mm. in 54 hours at 50°.0 
ped Ss Tw pa aia eee meter OO: 


This result is in perfect accordance with the observations of § 3. 


5. The following experiments prove in a more quantitative way 
that the previous thermal history of the metal has an influence on 
the transition temperature. 

A fresh quantity of the metal (4) was divided into two parts 
[(K,)r and (K,)77| of 500 grams each. 

(Kj. was reduced into turnings on a lathe and immediately put 
into a dilatometer. At 69°.9 we observed a decrease of volume 
(456 mm.) in 257/, hours. 

(K,)j) was converted into turnings in the same way and kept 
for 5 days and nights at 100° in a solution of cadmium sulphate. 

After having it put into a dilatometer (bore of capillary tube 1 mm.) 
we made the following readings (Table 1). 


TABLE I. 
| 

Temperature. Dee euaee ae \ Hee orth sib Beat: is 
hours. , in mm. per hour 

49.6 : — 100 | — 600 

60.4 ; — 125 — 250 

62.5 3 | ats ed 

63.1 ; ae its) + 45 

63.7 r + 83 | + 249 

69.6 " | + 225 | + 2700 


The transition point is 62°.8. 


6. The metal was now kept at 100° in contact with a solution 
of cadmium sulphate for 7 days and nights. After this it was put 


57 
again into a dilatometer which was heated for 24 hours at 145°, 
then for 24 hours at 270° (that is only 50 degrees below the melting 
point of the metal). 
We only succeeded in ‘bringing it into motion” by heating it for 
48 hours at 50° in a solution of cadmium sulphate. 
We then got the following results (Table IT): 


. TABLE Il. 

Duration of the Increase of the 

Temperature. observations in | pacueaee eae: level 
hours. : in mm. per hour 

° 

60.0 "Vo — 105 — 210 

63.0 ES — Il — 33 

63.5 | 1g — 8 | — 6 

64.0 | 11g | at 22 | ae 18 

| 
69.0 | Vg + 58 | + 348 


The transition point has been changed to 63°.4. 


7. In this way we carried out a great many experiments with 
samples of different previous thermal history *). The extreme limits 
which were found for this (apparent) transition temperature were 
69°.3 and 61°.3. 


8. As it is almost impossible to fix the real transition point 
of the pure modifications in this way, we tried to prepare a sharply 
defined modification of cadmium avoiding high temperatures. For 
this purpose we electrolyzed an ammoniacal solution of cadmium 
sulphate between an electrode of platinum and one of pure cadmium. 
(40 Volt, 20—25 Ampere ; surface of the electrodes 26 em?*.). 

We kept the temperature of the solution below 40°, cooling the 
vessel with ice. The solution was kept homogeneous by a glass-stirrer 
(Wirt), which was kept in motion by a small motor. The cadmium 
which was formed at the electrode was washed with dilute sulphuric 
acid, then with water, alcohol, and ether. After this it was dried at 40°. 

170 grams of this material were put into a dilatometer. As it is 
very finely divided, great care must be taken in order to remove the 
air from the dilatometer. We used a Garpr-pump for the purpose. 


1) The details will be given in full in our paper in the Zeilschrift f. physik. Ghem, 


58 


The paraffin oil was boiled on this pump with finely divided ead- 
mium. If there had been formed during the electrolysis only one 
modification of cadmium, we might expect that no transformation 
would occur in the dilatometer, in consequence of the absence of 
germs of a second form. From our earlier experiments (first paper 
§ 4) we know that even if a second modification were present the 
retardation may be very strongly marked. 

We found in our first experiment that neither at 50°, nor at 
80°, nor at 100° did any change occur. 

After having removed the paraffin oil we washed the metal with 
ether and brought it into contact with a solution of cadmium sul- 
phate (12 hours at 100°; 48 hours at 50°). After this the dilato- 
meter gave the following results (Table III). 


TABLE II. 
Téaperatuze | Digaiontoties. | Ieease obievel | dnsecas Oh a 
| 

71.0 | 34 — 351 — 468 
94.8 | Yq He5132 + 528 
70.5 | 53/4 — 267 = 5 
70.5 | i | Bea | ny 6 
60.0 24 | — 138 | — 6 
70.0 | 11), a7 0 + 46 
65.0 1p =) 853 | gs 


There is a change in the direction of motion of the meniscus at a 
constant temperature (7O°.5). The transition point is now between 
65 and 70°. 

This change proves therefore that now (viz. after the treatment 
at 100° and 50° with a solution of cadmium sulphate) there are 
simultaneously present more than two modifications. 


9. Finally it may be pointed out here that the pyknometer cannot 
be used to determine with exactness the density of the moditications 
of cadmium formed by electrolysis, as this material always includes 
constituents of the solution which has been electrolyzed. The water 
may be driven out by melting the metal; the salt will then flow 
on to the surface of the metal and may be washed away, but for 
exact determinations this material cannot be used. 


Utrecht, April 1914. van “tT Horr-Laboratory. 


59 


Chemistry. — “The allotropy of Zinc.” Il. By Prof. Erxsr Conny 
and W. D. HeLperMan. 


(Communicated in the meeting of April 24, 1914). 


1. In our first paper on the allotropy of zine’) we called attention 
to the “atomized” metals which may be prepared by the new method 
of M. U. Scnoop of Zurich. 

We then pointed out that this method forms an ideal way of 
producing chilled metal. As a result of our investigations on the 
metastability of the metals as a consequence of allotropy we may 
expect that ‘‘atomized” zine will contain two or more allotropic 
forms at the same time. 

From a technical standpoint we thought it interesting to prove 
this more directly : if the “atomized” metal really contains two or 
more modifications at the same time, it will disintegrate in the long 
run when stabilisation occurs. 


2. Mr. Scnoop supplied us with one kilo of zine, which had been 
“atomized” in the way described in our first paper on the subject. 
As the material is very finely divided one would expect that an 
eventual change would proceed in such a way that it could be 
measured easily. On the other hand much care must be taken to 
remove air from the very finely divided material after having brought 
it into the dilatometer. 


3. About 750 grams of the metal and a small quantity of glass- 
beads which had been heated beforehand*) were put into a dilato- 
meter. The material had not been in contact with an electrolyte. The 
capillary (bore 1 mm.) was bent horizontally and put in connection 
with a GarpE pump. In order to remove the air as completely as 
possible the dilatometer remained in connection with the pump 
for 1—1'/, hours. After this the paraffin oil was filled in; it had 
been carefully boiled on the pump at 200° in contact with some 
“atomized” zine. In this way the instrument was made perfectly 
free of air as many experiments proved. 


4. In a_ preliminary 


© 


of the metal occurs at 25°.0. We then carried out a fresh one, the 


experiment we found that a contraction 


“atomized” metal having been kept at 15° in a dry state for three 


1) These Proc. 16, 565 (1913). 
*) These Proc., 16, 485 (§ 10) [1913]. 


60 


months. We used a_ special thermostat, which will be before long 
described. The temperature was determined by means of a BrckMANN 
thermometer. It remained constant within some thousandths of a 
degree. 

The results are shown in Table I, 


TAUB LE we 
Temperature 25°.00. 


Level of the 
meniscus (mm.) 


Time in hours | 


0 526 
I 425 
22/, 252 
2/3 219 
112/5 181 


A strongly marked contraction at constant temperature occurs. 


5. As the metal contains a certain amount of zine oxide in 
consequence of its fine state of division, the question might arise 
whether the contraction observed may be attributed to some chemical 
reaction between the oxide and the paraffin oil. 

In order to investigate this point more closely we filled a dilato- 
meter (100 ec.) with zine oxide and the same paraffin oil we had 
used in the experiment described above. After having evacuated it 
at the GarpE pump we put it into a thermostat at 25°.00. The 
meniscus did not show any change in 24 hours. The contraction 
observed in our first experiment has consequently to be attributed 
to a change in the metal. We intend continuing our investigations 
on the different modifications of zine present in.the “atomized” metal. 


Utrecht, April 1914. vAN 't Horr-Laboratory. 


Chemistry. — “The allotropy of Copper’. UU. By Prof. Ernst Coney 
and W. D. Henperman. 


1. We have also continued our investigations on the allotropy 
of copper in the direction indicated in our second paper on the 
allotropy of cadmium. 

The dilatometer had shown (§ 4 of our first paper) that there is 
a transition point at 71°.4. We used the same method described in 
our second communication on cadmium in order to determine if 


61 


this point changes by a change in the previous thermal history of 
the metal. 


2. The sample the transition point of which had been fixed at 
71°.7 ($6 of our first paper) had not been treated with an electrolyte. 
It was removed from the dilatometer, washed with ether and kept 
in contact for some days with a solution of copper sulphate. This 
material (Cu,,) then gave the following results: 


TABLE I. 


| Duration of Rise of level 


Rise of level 


Temperature. measufements in | ie a ae 
61.7 ie | — 78 — 468 
14.6 | lg | 4.225 41350 
69.6 | Iq | 38 | — 152 
72.1 tg | + 67 | + 402 
70.3 | \poiassss [es 
11.6 2/5 + 84 4. 126 
70.8 | ip | Te aae | LL O7 
10.6 1g | — 10 — si 
70.7 | Big | 4. 36 fe 


The transition point has thus been altered from 71°.7 to 70°.65. 


3. As far as the measurements we carried out with samples of 
very different previous thermal history are concerned, we only 
mention here that we found as upper limit of the transition tem- 
perature 71°.7, as lower one 69 .2. *) 


4. We merely give here some details concerning a sample (Cuz) 
which had been made by mixing a certain weight of Cuyy (Transi- 
tion point 70°.65) with an equal anantity of the original material 
(Kupfer-KanLBaum, Elektrolyt, geraspelt), which as we were told 
when purchasing it, had heen melted after electrolysis. Curr had 
been at 50° for 10 days and nights in contact with paraffin oil. 
The results are given in table II. 


1) The description of our experiments will be given in full in our paper in the 
Zeitschr. f. physik. Chem. 


62 


TABLE II. 


Rise of level 


Tempertre. | gpumienest, | Rita | 
co ee 
68.0 21, = 5 | iG 
75.0 11/2 + 46 | + 30 
72.0 5/6 + 14 | Be iti 
70.0 5, + 10 | Me sy 
69.5 58 1-243 | Me 
69.5 31 — 36 | =a 


At constant temperature (69°.5) the direction of motion of the 
meniscus has changed. This change proves that also in this case 
there are more than two modifications present at the same time. 


5. How. extraordinarily marked the retardations are which may 
oceur, is shown by the behaviour of a sample Cury (comp. § 7 of 
our first paper); it was not possible to “bring it into motion” even 
after treating it with a solution of copper sulphate. However, it 
ought to be pointed out that there was no finely divided powder 
present, which was the case with the other samples we investigated. 


Utrecht, April 1914. van ‘t Horr-Laboratory. 


Botany. — “nergy transformations during the germination of 
wheat-grains’. By Luerm C. Dover. (Communicated by Prof. 
F. A. B.C. Went). 


(Communicated in the meeting of April 24, 1914). 


The reserve materials of seeds represent a large quantity of che- 
mical energy. In germination these substances are split into com- 
pounds with a much smaller number of atoms and partly by the 
process of respiration completely oxydized to carbon dioxide. In 
consequence of these exothermic processes a considerable quantity of 
energy is set free, which can be used for the various vital- 
processes. 

In order to obtain a conception of these transformations of energy 
during germination, | have made some observations on germinating 


63 


wheat-grains, on which I now wish to make a short preliminary 
communication. 

The germination of the wheat-grains under observation always 
took place at about 20° C. in the dark, there couid therefore be no 
energy taken up from without by assimilation of carbon dioxide ; 
all the energy needed for the processes of germination had therefore 
to be provided by means of the reserve materials. 

At the commencement of germination imbibition chiefly takes 
place, in this way heat is already liberated, therefore energy ; then 
there follow very soon a series of exothermic processes, in wheat- 
grains more especially decomposition of starch to sugars and com- 
plete oxydation of this material of respiration to carbon dioxide. 
The energy set free in this manner is now applied to various ends : 
1st. for all kinds of synthetic processes by means of which plastic 
materials are formed for the growing plant, 2". for the production 
of osmotic pressure, 3". for the overcoming of internal and external 
resistances, and 4'>. energy is given offin the form of heat-radiation. 

The methods used to obtain an insight into these various energy- 
relations were the two following : 

1s'. Determination of the heat of combustion before germination, 
and after the germination had been progressing for some time. 

2-4. Determination of the quantity of heat produced during ger- 
mination. 


As regards the first point, it must be pointed out that the internal 
chemical energy during a certain length of germination must decrease; 
a measure of this loss can be found by determining the difference 
in the heat of combustion. The energy which will no longer be 
shown by this heat of combustion, is that which is utilized osmoti- 
cally, for overcoming resistances and which is lost by the giving out 
of heat. The energy, however, which is used up during germination 
for synthetic processes is again fixed as chemical energy and is 
indeed represented by the heat of combustion. 

The loss of energy, that is found by determinations of the heat of 
combustion, does not give therefore the total amount of energy, 
which has played a part during germination, for a considerable part 
of this energy has again been withdrawn from observation by the 
synthetic processes. 

The Brrtue.ot-bomb was used for determining the heat of com- 
bustion. In it a weighed quantity of wheat-grains, germinated or 
ungerminated and previously dried for a long time at 100°, were 
burnt; by the rise of temperature of the water in which the bom 


64 


was placed, in combination with the water-value of the respective 
parts, the amount of energy which was set free by combustion, 
could be caleulated. 

This heat of combustion was always calculated for the weight of 1 
eram of ungerminated wheat (initial-weight) ; this was done in the case 
of both germinated and ungerminated wheat. In this way comparable 
values were obtained; the difference in heat of combustion after a 
definite period of germination gave therefore the loss of energy 
above referred to. 

Heat of combustion of wheat calculated per gram of the initial-weight, 


expressed in gram-calories. 


ee 


The germination took Average 
place at + 20° C. | | values | 


| | 
————— ———————— . 


Ungerminated 3748 — 3774 — 3778 —3794—3797!)| 3778 


Loss of energy ~ 


Sudtin; 0.6 Ist day 
After 1 day’s germin: 4 
Me wewic 2nd day 
meet ay ” 3756—3793 3774 ) 
lise OE eigemrenpaies 3rd day 
Pog : 3740 3740} 
? ; 94 4th day 
ye ey " 3653—3681—3682 —3707—3707 | 3686 j 
| ( Year O62 5th day 
” 5 » ” 3594 3594 | ) 
' OG). mentee 6th day 
” 6 ” ” 3498 3498 
180) eee Ith day 
” 7 ” ” 3318 3318 | 


It is clear from these values, which were found for the heat of 
combustion, that the loss of energy during germination steadily 
increased. The loss of energy in the first two days was slight ; 
probably imbibition had chiefly taken place at this stage, whilst the 
chemical transformations had then only subsidiary importance. 

It can be further deduced from the figures that between the 2"4 
and 38" day especially the loss of energy greatly increased, and after 
that continued to rise. 

If these values for the loss of energy after different lengths of 
vermination are summarized graphically, a curve is obtained, whieh 
begins almost horizontally, and rises more and more steeply. 

The loss of energy per hour per kilogram of initial-weight can be 
roughly ealeulated from the loss of energy during the different days. 

The loss of energy per gram of initial-weight was after two days 
4 calories. 


1) The figures are arranged in ascending values, and not chronologically. 


65 


During the 1s* and 2.4 days the loss of energy per hour per kilogram of 
g i 8. | $s 


1000 
the initial-weight was therefore roughly is = oom, cals 
LOOG 
The same for the 3'¢ day aie pq et ==141'7...;, 
9 ” ” ” 4th ” ” S< 54 —= 2250 as 
We. 2 Bees Ol aes su Jn S833 |, 
”? ” ” ” Gt ” ” << 96 — 4000 an 
” ” ” ”» oh ” ory < 180 SS 7500 5 


This amount of lost chemical energy corresponds therefore in all 
DO. 

probability to that which is applied to osmotic purposes, to the over- 

coming of resistances and to the evolution of heat. 


In a second series of observations | aiso attempted to determine 
directly the amount of heat that is given off. The principle, that 
underlay these determinations, was briefly as follows: air, saturated 
with water-vapour, which had been brought to a constant known 
temperature, was passed over germinating wheat-grains at a constant 
velocity ; these acted as a continuous source of heat; the air which 
passed over it therefore rose in temperature. 

If the difference of temperature between the air streaming in and 
out were measured, when the latter passed at a known rate, then 
in the ideal case when absolutely no other heat conduction took 
place, the amount of heat set free could be calculated from the 
known heat-capacity of the air. Moreover for this the space in which 
the seedlings were placed would have to be completely saturated with 
water-vapour ; if this were not so, evaporation would take place on 
germination, in whieh way heat would be withdrawn from the 
observation. 

The apparatus: with which | conducted these experiments consisted 
of a copper vessel placed in a waterbath of constant temperature. 
Through this copper vessel, in which a large number of germinating 
wheat-grains were placed, a current of air was directed at the rate 
of % litres per hour; the air had had for a large part of its course an 
opportunity to take up the constant temperature of the water. A set 
of thermal needles served to measure the difference between the tem- 
peratures of the air entering and leaving; the current resulting 
from this difference in temperature was led through a very sensitive 
mirror-galvanometer, whilst a spot of light was thrown by the mirror 
on a seale and so made it possible to compare accurately the deflections, 

The apparatus was for the most part composed of materials which 

0 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


bb 


conduct heat very easily, thus making the ideal case described above 
very far from being realised. 

If a source of heat were introduced into the vessel while a regu- 
lated stream of air was passed through, only a part of the heat 
liberated could be used to raise the air-temperature ; the remainder 
would pass into the surrounding water by conduction. 

It was to be expected that, when a definite source of heat was 
present, a maximum difference of temperature between the in- and 
out-sireaming air would arise after some time; with the given rate 
of passage of the air this difference of temperature caused by this 
source of heat, could not become greater. A calculation as to how 
ereat this maximum difference of temperature would be for different 
amounts of heat, would be very complicated, if not entirely impos- 
sible. For this reason the simplest way was to calibrate the apparatus 
by introducing a source of heat of known magnitude. For this 
purpose a manganin-wire was placed inside the apparatus over as 
wide an extent as possible, in the place where later the germinating 
wheat-grains were to be put. This wire formed a metallic contact 
with two copper rods which projected above the lid of the appara- 
tus. An electric current could be passed through the manganin-wire 
by connecting these rods with the two poles of an accumulator. 
The resistance of the manganin-wire was accurately determined, whilst 
a milliamperemeter, placed in the cireuit, served to measure the 
strength of the current. By taking the current from 1, 2, and 3 
accumulators alternately, sources of heat of different magnitude could 
be introduced into the apparatus. 

When in this way a source of heat of known magnitude occupied 
the apparatus, air was passed through and at regular intervals the 
(double) deflection of the spot of hght on the scale was read till 
this ultimately remained constant and therefore had reached a 
maximum. These observations were conducted at temperatures of 
20°, 30°, and 40° of the surrounding water, and also therefore of 
the entering cr. 

These calibration-experiments showed: 1st that the maximum 
deflection of the spot of light, or in other words the difference of 
temperature between the in- and out-going air was roughly in 
proportion to the source of heat which was placed in the apparatus, 
2e¢ that this proportionality was maintained at a surrounding 
temperature of 20°, 30°, and 40°, 3" that the absolute magnitude 
of the deflection was independent of this temperature, 4'", that a 
deviation of 1 centimetre corresponded to a development of about 


11.5 calories per hour. 


67 


As the apparatus was now calibrated it was possible conversely, 
by reading the deflection of the spot of light, to calculate the 
magnitude of any source of heat, which was in the apparatus. For 
such an unknown source of heat germinating wheat-grains were 
used. (The number of these was always 500). 

In the course of the experiments however it became plain that 
in this ease the deflection of the light spot could not be looked 
upon as showing exclusively the heat-evolution which took place in 
germination. For when 500 germinated wheat-grains, which had 
previously been killed by heating to 106°, were placed in the 
apparatus, then it was seen that the spot of light inevitably 
passed the zero; in various experiments of this kind a deflection of 
about 8 centimetres was always found. 

In order to ascertain whether the dead seedlings did not after 
all give off some heat possibly as a result of a continued enzyme- 
action, the apparatus was filled by way of control with quantities 
of filterpaper previously soaked in water. In this case there could 
be no question of heat-evolution by the filterpaper. Also with this 
arrangement of the experiments the spot of light invariably passed 
the zero, reaching finally a maximum deflection corresponding to 
that obtained when dead seedlings were placed in the apparatus. 
The extent of this deflection was independent of the temperature of 
the surrounding water (fixed at 25° and 35°), in other words, with 
this arrangement of the experiment there arose always a constant 
difference of temperature between the in- and out-going current of air. 

Since in these cases no direct evolution of heat by means of the 
substances used was possible, another cause for the rise of temperature 
in the experiment described had to be found. The most probable 
thing was that condensation of water-vapour must have taken place 
in some way and that the heat thus set free caused an increase of 
temperature in the out-going air and in consequence of this of the 
upper thermal needle. In the calibration-experiments the spot of 
light had remained at zero when there was no heat-source in the 
apparatus; the difference in conditions then and during the experiments 
just described was, that the space within was in the latter case for 
a great part filled with a completely imbibed mass. 

The many efforts made to eliminate this irregularity were practically 
without results; I was therefore compelled, in experimenting with 
living seedlings, to adopt a correction, the amount of which was 
experimentally fixed while theoretically it had to be left partly 
unexplained, 

Since it was therefore found that by filling the apparatus with 

58 


b8 


very moist substances a difference in temperature between the two 
needles arose when the current of air passed through, it had to 
be assumed that this would be also the case when living seedlings 
were present. The deflection found in that case would have to be 
attributed partly to this physical cause, partly to generation of heat 
which actually took place in germination. It was therefore necessary 
to subtract from the deflection found in this arrangement the amount 
of deflection found in the experiments with dead seedlings, the 
remainder then being the measure of the heat generated in germination. 
This latter was observed at different temperatures and in different 
stages of germination. In consequence of the complications mentioned 
higher up the sources of error were relatively very numerous’ and. 
this was. especially noticeable in’ the few parallel-determinations 
which were carried out, so that in the values summarized in the 
table below an approximation to the amounts of heat given off 
must be expected rather than an exact measure thereof. These 
influences are proportionately very large in the lower values. 


Number of calories given off per hour calculated per kilogram 
of the initial weight. 


eee 


| | | | 
a. | On the 2nd} On the 3rd | On the 4th | On the 5th | On the 6th | On the 7th 
5 day of | dayof | day of day of day of | day of 
f | germination) germination germination | germination | germination | germination 
| | | | 
20° | 710 "2143 2790 | 2869 
: : : St is | ates 
25° 363 540 | 2938 2977 4341 
3455 
30° | | | 4999 «| = 6790 | 
6313 
Boe 752 7326 | 71575 
| 
io MiMi se | - 
40° | | 5689 6847 


It appeared therefore from the values found that the generation 
of heat on the 2™¢ and 3° days was still small in comparison to 
that in later stages of germination. The generation of heat shows 
a great and sudden increase between the 3'¢ and 4 day and it 
is probable that it continued to increase slowly during the following 


69 


days, but the relatively small differences from the 4 to the 7! day 


justify the calculation of an average for this period of germination. 


Number of calories given off per hour calculated per kilogram 


of the initial weight. 


The generation of heat, therefore, 


surrounding temperature; by arise 


Temp. leery aa 5th day | 6th day | 7th day, Average 
20° 2143 | 2790 | 2869 2601 
| 
| harness | 
25° | 2038 | 2977 | 4341 3428 
| 3455 | 
30° 4999 | 6790 | | 6034 
6313 | 
| 
35° 7326 | 7575 | 7450 
——— + — ~~ —~ 
40° | 5689 | 6847 6268 
| | | 


was much influenced by the 
of 10°, the quantity of heat 


evolved, increased to more than double. The generation of heat was 


diminished at 40°, a proof of the harmful influence of this temperature. 
| | 


Finally a comparison can be made between the number of calories 


pro kilogram of initial weight given 


off as heat and the loss of 


energy deduced from the heat of combustion. This comparison could 


only be made for a temperature of 20° 


because at this temperature 


germination had always taken place, so that the heat of combustion 
referred to processes at this temperature only, 


Loss of energy per hour per kilogram of the initial weight. 


At 20° By heat given off 


On the 2nd day | 


' Calculated from the 
| heat of combustion 


83 Cal. 
f4i7' . 


py oils 710 Ca. 
ee ee 4th 3 2143, 

Sy iw eOUnue 5 2790 , 

re pa Melos a 

en i pithien 2869 , 


2250, 


3833 
4000 
7500 


70 


The total amount of chemical energy which was set free in 
evermination was therefore always larger than the quantity of energy 
given off as heat to the surroundings. A part of the free energy 
which became available in the process of germination was therefore 
evidently used for other purposes (osmosis ete.) than for heat-evolu- 
tion only. 

This was however doubtful only on the second day, the evolution 
of heat on that day was not determined; the loss of energy, cal- 
culated from the heat of combustion, was however so small in this 
period that it is very possible that the evolution of heat at that 
moment was larger. If afterward it should appear that this is really 
the case, it would be very intelligible. For in the beginning of 
germination imbibition will principally take place so that in this 
case evolution of heat is not at all necessarily connected with chemical 
transformations. 

The results of this investigation may therefore be summarized 
as follows. 

The loss of energy calculated from the heat of combustion as 
well as the evolution of heat increase with the duration of germination. 

Both are small at the beginning of germination and greatly increase, 
chiefly on the 34 day. 

The evolution of heat is greatly dependent on the surrounding 
temperature. 

The optimum of beat-evolution is roughly 35°, 

The total loss of energy during germination at 20° exceeds the 
loss of energy by evolution of heat at the same temperature. 


Utrecht, 1914. Botanical Laboratory. 


Chemistry. — “Lyquwilibria in ternary systems XV”. By Prof. F: 


A. ,H. SCHREINEMAKERS. 
(Communicated in the meeting of April 24, 1914). 


In our previous considerations on saturationcurves under their own 
vapourpressure and on boilingpointeurves we have considered the 
veneral case that each on the three components is volatile and 
occurs consequently in the vapour. Now we shall assume that the 
vapour contains only one or two of the components. Although we 
may easily deduce all appearances occurring in this ease from the 
general case, we shall yet examine some points more in detail. 


The vapour contains only one component. 

We assume that of the components A, 6, and C' the first two 
are extreiaely little volatile, so that practically we can say that the 
vapour consists only of C. This shall e.g. be the ease when A and 
/ are two salts and Ca solvent, as water, alcohol, benzene, ete. 

Theoretically the vapour consists always of A+ B+ C; the 
quantity of A and 4, however, is generally exceedingly small, 
compared with the quantity of C, so that the vapour consists prac- 
tically completely of C. 

When, however, we consider complexes in the immediate vicinity 
of the side AZ, circumstances change. A complex or a_ liquid 
situated on this side has viz. always a vapourpressure, although 
this is sometimes inmeasurably small; consequently there is also 
always a vapour, consisting only of A+ 45 without C. When we 
take a complex in the immediate vicinity of the side AZ, the 
quantity of C' in the vapour is, therefore, yet also exceedingly small 
in comparison with the quantity of A+ Sb. 

Considering equilibria, not situated in the vicinity of the side 
AB, we may, therefore, assume that the vapour consists only of C; 
when, however, these equilibria are situated in the immediate 
vicinity of the side AA, we must also take into consideration 
the volatility of A and # and we must consider the vapour as 
ternary. 

Considering only the oceurrence of liquid and gas, as we have 
formerly seen, three regions may occur, viz. the gasregion, the 
liquid-region and the region L—G. This last region is separated from 
the liquid-region by the liquid-curve and from the vapour-region 
by the vapourcurve. 

As long as the liquid-curve is not situated in the immediate 
vicinity of AZ, this last curve, as a definite vapour of the vapour- 
curve is in equilibrium with each liquid of the liquid-curve, will 
be situated in the immediate vicinity of the anglepoint C. Therefore, 
the gas-region is exceedingly small and is reduced, just as the gas- 
curve, practically to the point C. Consequently we distinguish within 
the triangle practically only two regions, which are separated by the 
liquid-curve, viz. the liquid-region and the region L—G ; the first 
reaches to the side AZ, the last to the anglepoint C. The conjugation- 
lines liquid-gas come together, therefore, practically all in the point C. 

When, however, the liquid-curve comes in the immediate vicinity 
of the side AA, so that there are liquids which contain only exceed- 
ingly little C, then in the corresponding vapours the quantity of 
A and & will be large with respect to C. The vapour-curve will 


72 


then also be sitnated further from the anglepoint C and closer to 
the side AB, so that also the vapour region is large. At a sufficient 
decrease of pressure or increase of temperature, the vapour-region 
shall even cover the whole components-triangle. Consequently it is 
absolutely necessary that we must distinguish the three regions, of 
which the movement, occurrence, and disappearance were already 
formerly treated. 


When the equilibrium “+ 2+ G occurs, we may now deduce 
this in the same way as it was done formerly for a ternary vapour. 

a) The solid substance is a ternary compound or a binary com- 
pound, which contains the volatile component C. 

For fixing the ideas we shall assume that in the triangle ABC 
of fig. 1 which is partly drawn, the point C’ represents water, /’an 
aqueous doublesalt, #4” and /” binary hydrates. In accordance with 
our previous general deductions we now find the following. 

The saturationcurves under their own vapour-pressure are circum- 
or exphased at temperatures below 7’, (7’,—= minimum meltingpoint 
of the solid substance under consideration). The corresponding vapour- 
curves are reduced to the point C. When these substances melt with 


Fig. 1, 
increase of velume, the points //, H’ and //’ are situated with 
respect to /, #”’ and F" as in fig. 1; when they melt with decrease 


of volume, these points are situated on the other side. 


73 

In fig. 1 different saturationcurves are completely or partly drawn ; 
the pressure increases along them in the direction of the arrows. 
Further it is apparent that along the saturationcurve of /’ the pressure 
is maximum or minimum in its points of intersection with the line 
CF; the point of maximumpressure is situated closest to C. On 
the curve bcdihg of fig: 1, which is only partly drawn, c is, 
therefore, a point of maximum-, 4 a point of minimumpressure. 

The pressure along a saturationcurve of the binary hydrate /” 
(or #'") is highest in the one and lowest in the other end, without 
being however in these terminating points maximum or minimum. 
On the curve abg/f of fig. 1 which is only partly drawn, the 
pressure in @ is the highest and in / the lowest. 

This is also in accordance with the rule, formerly deduced, that 
the pressure is maximum or minimum, when the phases /’, 4, and ( 
are situated on a straight line, but that this is no more the case 
when this line coincides with a side of the triangle. 

As the vapour has always the composition C here the point of 
maximum- and that of minimumpressure of the saturationcurve of / 
are, therefore, always situated on the line C#’; the saturationcurves 
of F’ and F" can, however, not have a point of maximum- or 
minimum-pressure. 

As we may obtain all solutions of the line Ch (CB and CA) 
by adding water to / (F” and F'") or removing water from /’ (/” 
and F'"), we shall call the solutions of Ch (CB and CA) pure 
solutions of # (#” and Ff"). Further we eall the solutions of C H/ 
(CH’ and CA") rich in water and those of Hh (H’B and H"A) 
solutions poor in water. Consequently in fig. 1 a, ¢ and e represent 
pure solutions rich in water and f, 4 and & pure solutions poor in 
water. We may express now the above in the following way : 

Of all solutions saturated at constant 7’ with a binary or ternary 
hydrate, the pure solution rich in water has the greatest and the 
pure solution poor in water the lowest vapourpressure. Therefore, 
the pressure increases along the saturationcurve from the pure solution 
poor in water towards the pure solution rich in water. When the 
solid substance is a ternary hydrate, the highest pressure is at the 
same time a maximum- and the lowest pressure also a minimum 
pressure, 

We see that this is in accordance with the direction of the arrows 
Vay jot Ale 

6) The solid substance is the component A or / ora binary com- 
pound of A and £4; therefore, it does not contain the volatile com- 
ponent C. 


7+ 


In fig. 2 some saturationcurves under their own vapourpressure 
of A (ak, blem,on) and of B (hi,g lfm, pn) are completely or 
partly drawn. When in one of the binary systems, e.g. in CB, there 
exists a point of maximumtemperature H’, then also there occur 
saturationcurves as the dotted curve gi. As long as we consider 
solutions, not situated in the vicinity of AB, the vapour region is 
represented by point C. When we consider, however, also solutions 
in the vicinity of A 4, the vapour region expands over the triangle. 
Consequently, when we de- 
duce the — saturationeurves 
under their own vapour-pres- 
sure, assuming that the 
vapour is represented by C, 
we may do this only for 
solutions, not situated in the 
vicinity of AB. For points 
of the curves in the vicinity 
of AL we take the case, 
treated already in communi- 
cation XIII that the vapour 
is ternary. The same applies, 
as H’ is situated in the vicinity of 5, also to the curves in the 
vicinity of H’. 

If follows from the deduction of the saturationcurves that the 


pressure, e.g. along a, continues to decrease from a; only in the 
vicinity of 2, a point of minimumpressure may perhaps be situated. 
As the pressure in 6 and consequently also in the minimum possibly 
occurring is exceedingly small and practically zero, we can say: 
along tae saturationcurve of a component the pressure increases 
from the solution free from water (4) towards the pure solution (q). 
The pressure of the solution free from water is practically zero. 

Let us now take a binary compound of A and # (for instanee 
an anhydric double-salt); it may be imagined in fig. 2 to be repre- 
sented by a point # on AL. When we leave out of account satura- 
tioncurves in the vicinity of #, we may say that the saturation- 
curves under their own vapourpressure have two terminatingpoints, 
both situated on AS. As the pressure is again very small in both 
the {terminatingpoints, it follows: along the saturationcurve of an 
anhydric doubdle-salt, the pressure increases from each of the solutions 
free from water towards the pure solution. 

c) The solid substance contains the volatile component C' only. 

This is for instance the case when an aqueous solution of two 


io 


salts is in equilibrium with ice; the saturation- or icecurve under 
its Own vapourpressure has then, as curve ed in fig. 2, one ter- 


ay 


minatingpoint on C A and one on C4. We find further: along an 


icecurve under its Own vapourpressure the pressure is the same in 
all points and it is equal to the pressure of sublimation of the ice. 


We may deduce the previous results also in the following way. 
As the vapour consists only of C, we equate, in order to find the 
conditions of equilibrium for the system /-+ 4+ G in (1) (Il) 
Zo—OLand 7v— 0. We then find: 

OZ 


Lb 


Z—3 


Z IZ WA 
a eet and Z.-pe. apipey sr aa Fey se ee GL) 
y 


For the saturationcurve of / under its own vapourpressure we 
find : 

(Gop saa (Gist) O,j—— Giddens by (2) 

(art Bs\de+t(astBddy=—(A+tOdP .. .¢ 

which relations fellow also immediately from 8 (II) and 9 (II). In 


order that the pressure in a point of this curve should be maximum 
or minimum, dP must be = 0. This can be the case only, when 


COP SS MRS oe ee ere eo (GH) 


This means that the liquid is situated in the point of intersection 
of the curve with the line CF’, consequently, that the liquid is a pure 
solution of /’. Consequently we find: along a saturationcurve under 
its Own vapourpressure of a ternary substance, the pressure is 
maximum or minimum in the pure solutions. 

In order to examine for which of the two pure solutions the 
pressure is maximum and for which it is minimum, we add to the 
first part ef (2) still the expressions : 


1 Or 108 1 Or Os snd : Ose SOL sy? 
3’ pas +y = a 1 (stots I, 7) vdy +-— 2( 1 Lo 5, } ye. 


and to the first term of (38): 


1 Or ac is ony ate Pedy 1 Ose me ee 
3 Biv + | a da~ +- oy +- { a dudy +4 9 («5. + | 5.) dy? + 


. 


Now we subtract (2) from (3), after that (2) is multiplied by «& and 
(3) by w. Substituting further their values for A and ¢ 


" we find: 


1 
5 (rda* +- 2sdedy + tdy’) = [(e—a) V, + a V—avjdP. . (5) 


ra 


Representing the change of volume, when one quantity of vapour 


76 


arises at the reaction between the phases F, LZ and G, by AV, 
(5) passes into: 

1 

5 @(rde* 4 Asdady + tdy*) = (c—a) AV, X<adP a un) 

Let us consider now in fig. 1 the pure solutions of F, therefore - 
the solutions of the line Ch. For points between Cand f «—a<0, 
for the other points «2 —e > 0. Considering only the solutions of 
the line Ch, we can consider the system “+ L-+ G as binary. 
Imagining a P,7-diagram of this system, // is the point of maximum- 
temperature. From this it is apparent that AV, is negative between 
H and F, positive in the other points of the line Ch. From this it 
follows: : 

(e—a) AV, is negative in points between C and H, therefore for 

the solutions of /” rich in water. 

(a—a) QV, is positive in the other points of this line, therefore, 

for the solutions of /° poor in water. 

The same applies also when the point // is situated on the other 

side of 

Let us take now a pure solution rich in water of /’, for instance 
solution c of the fig. 1; as the first term of (6) is positive and 
(a—a) AV, is negative. it follows: dP is negative. This means that 
the pressure is a Maximum in ¢. 

When we take a pure solution poor in water of /’, for instance 
solution h of figure 1, (e—a)AV, is positive, therefore, the pressure 
is a minimum in h. 

In accordance with the previous considerations, we find, there- 
fore, that the pressure along the saturationcurve of a ternary com- 
pound is a minimum for the pure solution poor in water and a 
maximum for the pure solution rich in water. 

When the solid substance is a binary compound, as /” in fig. 1 
or 3, we must equate «=O. (Of course 3 =O for the compound 
F’"). (2) and (3) pass now into: 

(wr + ys) dx + (as + yt)dy=-—CdP . . . 2) 
Bsda + pidy = —(A + @)\dR, 2 2 es) 

From this we find: 

Bu (rt — s*) da =[(as + yt)(A + C) —BC))dP . . . (9) 

From this it is apparent that dP? can never be zero or in other 
words: on the saturationcurve of a binary hydrate never a point of 
maximum- or of minimumpressure can occur. 

In the terminatingpoint of a saturationcurve on BC« =0; as 


j 7 
Lim it while ¢ and s remain finite, it follows, when we 
& 
replace also A and C' by their values: 
Bee da — || — 8) Veep —yoee. s 2=. (10) 

Representing by AV, the change of volume, when one quantity 
of vapour arises at the reaction between the three phases (#”, L 
and (G), (10) passes into: 

BRL edec — (y — PB) A VeriOve b= gee eeeaNes. 6 (1h) 

For solutions between C and /” is y— <0, between /” and 
B is 1—gs>O0. Imagining a P,7-diagram of the binary system 
hr t+L+G, H’ is the point of maximum temperature; A’, is 
consequently negative between //’ and /”, positive in the other 
points of C4. From this it follows: (y — Bp) AV, is negative in points 
between C' and //’, therefore, for the solutions rich in water; (y—~) 
AV, is positive in points between //’ and #, therefore for the 
solutions of #” poor in water. 

From (11) it now follows: dP is negative for liquids on CH’, 
positive for liquids on H’. In accordance with our former results 
consequently we find: along the saturationcurve of a binary hydrate 
the pressure increases from the pure solution poor in water towards 
the pure solution rich in water. 

When /° is one of the components, which are not volatile, e.g. 
B in fig. 2, then a=O and B=1. From (11) then follows: 

RT .d«e =(y — NN AWA 5 CHE arama oo (12) 

We now imagine a P,7-diagram of the binary system B+ 1+G; 
this may have either a point of maximumtemperature //’ in the 
vicinity of the point 4 or not. When a similar point does not exist, 
AV, is always positive; when a similar point does exist, AV, is 
positive between C’ and #1’, negative between H’ and B. As we 
leave, however, here out of account points, situated in the vicinity 
of B, AV, is positive. As y—1 is always negative, it follows 
from (12) that dP is negative. In avcordance with our former results 
we find therefore: along the saturationcurve of a component the 
pressure decreases from the pure solution towards the solution free 
from water. 

When F is the volatile component, as for instance in the equili- 
brium tce+ L+G, then «=O and B=O. The second of the con- 
ditions of equilibrium (1) passes now into: Z =. This means that 
not a whole series of pressures belongs to a given temperature, but 
only one definite pressure, viz. the pressure of sublimation of the 
ice. Therefore we find again: along an icecurve under its own 


ke) 


Vapour pressure the pressure is the same in all points and equal to 
the pressure of sublimation of the ice. 


Now we shall consider the boilingpointcurves; in general the 
same applies to them as to the saturationecnrves under their own 
vapourpressure, which we have considered above. 

Now we assume that the curves in fig. 1 represent boilingpoint- 
curves; the point /7 no longer represents a point of maximum 
temperature, but a point of maximum pressure ; consequently it is 
always situated between C and #. This point of maximumpressure 
His always situated closer to C' than the point of maximum tem- 
perature /7; the same applies to the points #7’ and #" in the figs. 
2 and 8. Wishing to indieate by arrows the direetion in which the 
temperature increases, we must give the opposite direction to the 
arrows in the figs. 1—3s. 

We saw before that on the side CB of fig. 2 a point of maxi- 
mumtemperature /7/’ may either occur or not; on this side, however, 
always a point of maximumpressure is situated. The same applies 
to the side C'A. We now find the following. 

a) of all solutions saturated under constant P with a binary or 
ternary hydrate, the pure solution rich in water has the lowest — 
and the pure solution poor in water the highest boilingpoint. There- 
fore, the boilingpoint inereases along the boilingpointeurve from the 
pure solution rich in water towards the pure solution poor in water. 
When the solid substance is a ternary hydrate, the highest boiling- 
point is at the same time a maximum- and the lowest at the same 
time a minimumboilingpoint. 

6) along the boilingpointeurve of a component or of an anhydrie 
double-salt the boilingpoint increases from the pure solution. When 
the solid substance is an anhydrie double-salt, the boilingpoint of 
the pure solution is at the same time a minimum. 

c) along the curve of the solutions saturated with ice under a 
constant pressure the boilingpoint is the same in all the points and 
it is equal to the sublimationpoint of the ice. 

The icecurve under its Own vapourpressure of the temperature 
7’ and the boilingpointeurve of the ice under the pressure P coincide, 
therefore, when / is the pressure of sublimation of the ice at the 
temperature 7. 


The following is amongst others apparent from what precedes. 
We take a pure solution of a solid substance (component, binary or 
ternary compound). Through this solution pass a saturationcurve 


Us) 


under its Own vapourpressire and a boilingpointcurve. Generally we 
now have: when the vapour pressure at a constant 7’ decreases (or 
increases) from the pure solution, the boilingpoint under a constant 
P will increase (or decrease). 

This, however, is no more the case for solutions between the 
point of maximumpressure and the point of maximumtemperature. 
The point of maximumpressure is situated viz. closer to the point 
C than the point of maximumfemperature. When we take a solution 
between these points, it is a solution rich in water with respect to 
the saturationcurve under its own vapourpressure, & solution poor 
in water, however, with respect to the boilingpointeurve. Consequently 
as well the pressure along the saturationcurve as the temperature 
along the boilingpointcurve will decrease from this solution. 

We may express the foregoing also in the following way: the 
vapourpressure (at constant 7’) and the boilingpoint (ander. constant 
P) change from a pure solution generally in opposite directions. 
When, however, the pure solution is situated between the point of 
maximumpressure and the point of maximumtemperature, then as 
well the vapourpressure as the boilingpoint decrease from this solution. 


Formerly we have already considered the saturationcurve under 
its Own vapourpressure of two solid substances (viz. the equilibrium 
P+ Fk’ + L+ G); now we shall discuss some points more in detail. 
It should be kept in niind in this ease that all deductions apply 
also now to points, which are not situated in the vicinity of AB. 
The deductions discussed already formerly apply to points in the 
vicinity of this line. 

Let us take the solution m of fig. 2 saturated with A+B, ihere- 
fore, the equilibrium A+ 6-+ Z,,-+ G. As the pressure increases 
from m towards ¢ and towards /, we may say: the solution saturated 
with two components has a smaller vapourpressure than the pure 
solution of each of the components separately. 

When we consider the solution p of fig. 2 saturated with ice +A 
and when we imagine curve np to be extended up to CA, it appears: 
the solution saturated with 7ce-+ A has a greater vapourpressure 
than the solution saturated with A—+ / and a smaller vapourpressure 
than the metastable pure solution of A. 

In the previous communication we have already discussed the 
curves zu, 2v,and zw; 2 represents the solutions of the equilibrium 
A+65+L+G, zw those. of the equilibrium tee + A+ L+ G 
and zv these of the equilibrium tce+ B+ + G, w and v are 
binary, < is the ternary eryohydric point under its own vapourpressure. 


50 


Let us now contemplate the solution m of fig. 3 saturated with 
the hydrates 7+ /”; it is apparent from the figure that solution m 
has a smaller vapourpressure than 7 or n. When we take however 


Cw wn eek aa Cc 


the solution 4, saturated with these hydrates, this has a larger 
vapourpressure than the solutions @ and ce. 

Curve pq represents the solutions of the equilibrium #4 #”-++-L-+G; 
point HZ is the point of maximumtemperature of this curve. In 
accordance with our previous definitions we call the liquids of branch 
pH vich in water and those of branch //q poor in water. We then 
may express what precedes in this way: 

the solution saturated with two components or with their hydrates 
has in the region rich in water always a smaller vapourpressure, 
in «he region poor in water always a greater vapourpressure than 
the pure solution of each of the substances separately. 

Let us now take a liquid saturated with a double salt and one 
of its limit-substances. [In fig. 1 the series of solutions saturated 
with /’ of curve bed is limited in 6 by the occurrence of F” and 
in d by the occurrence of /'". Therefore we shall call 7” and #" 
the limit-substances of the double-salt /’). Curve po represents the 
solutions of the equilibrium /’-+ 4” + L-+ G, curve og those of 
the equilibrium #” + F+ + G and curve o7 those of the equili- 
brum F"+F+4+2-+G. M and M’ are points of maximum- 
temperature of these curves. In accordance with previous definitions 
we call solutions of o//7 and oJ’ rich in water and those of Mg 
and J//7 poor in water. 


81 


The following is apparent from the direction of the arrows in 
how AP 

a. In the region of the liquids rich in water. When a doublesalt 
is soluble in water without decomposition, the solution saturated 
with this double-salt and with one of ifs  limit-substances has a 
smaller vapourpressure than the pure solution of the doublesalt and 
also than that of the limit-substance. 

When a double-salt is decomposed by water, the solution saturated 
with this double-salt and one of its limit-substances has a smaller 
Vapour pressure than the pure solution of the limit-substanece. The 
solution saturated with double-salt and with the limit-substanee, which 
is not separated, has a smaller vapour-pressure than the solution, 
saturated with double-salt and with the limit-substance, which is 
separated. 

6. In the region of the liquids poor in water the opposite takes 
place. 


As a special case a liquid can be saturated with two substances 
of such a composition, that one of these may be formed from the other 
by addition of water. They are 
represented then by two points /” 
and #”, which are situated with C 
on a straight line. In fig. 4 this line 
CF does not coincide with one 
side of the triangle. In this figure 
aec f is a saturationcurve under 
its Own vapourpressure of /’, curve 
bedf one of F’; the arrows 
indicate the direction, in) which 


the pressure increases. Both the 

Fig. 4. curves can be circum- or exphased 
and they either intersect or they do not. In fig. 4 they intersect 
in e and f/f, so that the equilibria #” + #” + L. + G and 
F+ Ff’ + Lr+G occur. Now we can prove that the vapour 
pressure of those two equilibria is the same, therefore P= Pr. 
When we remove viz. the liquid from both the equilibria, we retain 
r+ Fk’ +G. As between these three phases the reaction */’+G 
is possible, we can consider /’+ #” + G as a binary system. We 
then have two components in three phases, so that the equilibrium 
is monovariant. At each temperature /’+ /” +- G has, therefore, 
only one definite vapourpressure, from which immediately follows : 
ips ad ee 

6 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


82 


Curve gehfk in fig. 4 indicates the solution of the equilibrium 
FtrF+t+L+G; when in a P, 7-diagram we draw‘the curve 
r+ F’ + G@ (consequently the curve of inversion /Z /” -+ G) and 
eurve /} + 7” + L+ G, then they coincide. 

In fig. 5 the line CFF” coincides with the side BC of the triangle ; 
We assume viz. that the component B and its hydrate /” occur as 
solid substances; further we have also assumed that the component 
A occurs as solid substance. The curves be, fy and th are saturation- 
curves under their own vapourpressure of A, th and ef of B, ab 
and de of the hydrate /’; the arrows indicate again the direction 
in which the pressure increases. 

It is apparent from the figure that vz represents the solutions of 
the equilibrium A+ /+ L4G, cw those of A+B+L+4G 

B and zu those of b+ F+4+L-+4G. 
Consequently in 2 the invariant equili- 
w brium A+ 6+ F+ 2+ 4 occurs. 
; Curve zu terminates on side BC in 
the quadruplepoint a with the phases 
B+ F+4 L+G of the binary system 
CB. When we remove the liquid LZ, 
from the equilibrium 5+ #7+21,+G 


occurring at the temperature 7, and 


C A underthe pressure /’., we retain the mono- 

(w) a variant binary equilibrium B+ 7G. 

Fig. 5 When we draw in a P,7-diagram the 

curve b+F+-G (therefore the curve of inversion / 2 5+-G) and 
curve B+ f+ L+G, these two curves coincide. We can say, 
therefore : 

the vapourpressure of a solution, saturated with a component and 
with its hydrate, is equal to the pressure of inversion of the hydrate 
(the pressure of the reaction 2 b-+ G). 

From the direction of the arrow on de it follows that the pressure 
in @ is smaller than in d. We can say, therefore : 

the solution saturated with a component and with one of its 
hydrates has a lower pressure than the pure solution of the hydrate, 

The same considerations apply also when two hydrates of a same 
component occur. 


We may summarise the previous results in the following way. 
Through each solution saturated with two solid substances go two 
saturationcurves; when we limit ourselves to the stable parts of 


83 


these curves, we may say that two saturationcurves proceed from 
such a solution. Then we may say : 

1. The two solid substances are situated in opposition with respect 
to the line LG. 

a. The solution saturated with these substances is rich in water: 

The pressure increases from this solution along the two satura- 
tioncurves. 

6b. The solution saturated with these substances is poor in water. 
The pressure decreases from this solution along the two saturation- 
curves. 

2. The two solid substances are situated in conjunction with 
respect to the line LG. 

a. The solution saturated with these substances is rich in water. 

The pressure decreases from this solution along the saturation- 
curve of that solid substance which is situated closest to the 
line LG; the pressure increases along the other saturationcurve. 

6. The solution saturated with these substances is poor in water. 

The same as sub 27.; we must take however the changes of 
pressure in opposite direction. 

3. The two solid substances are situated on a straight line with 
the vapour. 

The pressure increases from the solution saturated with these sub- 
stances alone the saturationcurve of the substance with the largest 
amount of water, it decreases along the saturationcurve of the sub- 
stance with the smailest amount of water. 

We find examples of 1¢ in the equilibria : 

FAR +1,+G (fig 1), F+F"+014+4 (fig. 1), A+B+L,+G4 
(figs. 1 and 2), #”+F"-+L,,4+G (tig. 3), A+ B+ ,4G4 (fig. 5) and 
F+A+L;/+G (fig. 5). 

We find examples of 1° in the equilibria: 7-+-/”’+-L,+4G (tig. 

Feu ae et Ga(fies 2) and. P42" by iG (fe. 3): 

An example of 2“ is found in the equilibrium /-+- /”+ L,+-G (tig. 1). 

We find examples of 3 in the equilibria: P+/”+21,.4-G (fig. 4), 
P+’ +Ljy+G (fig. 4) and B4+4+1,4 G (fig. 5). 

. 


We may deduce the above-mentioned rules also in the following 
way. We shall viz., while the temperature remains constant, change 
the volume of the system M+ /” + L4G, so that a reaction 
takes place between the phases and there remains at last a three- 
phase-equilibrium. As this reaction is determined by the position of 
the four points with respect to one another, we may immediately 
distinguish the above-mentioned cases 1, 2, and 3. When we eall 

6* 


S4 


the change of volume, when one quantity of vapour is formed at the 
reaction, AJV,, then AJ, is always positive, except when the 
liquid is represented by a point of the fourphase-curve between the 
point of maximumtemperature and the intersectingpoint of this curve 
with the line #/”.-When we now apply the rule: ‘the equilibria, 
which arise at increase (decrease) of volume, are stable under lower 
(higher) pressure’, we may easily refind the above-mentioned rules. 

When we take as an example fig. 38 in which the case sub 1 
occurs, the equilibrium /” + /".+ L + G is represented by curve 
pq, Which intersects the line A’ 7" in WS; 7 is the point of maximum- 
temperature of this curve. Consequently 4’ is positive on pH and 
Sq, negative on //S; the solutions of p/ are rich in water, those 
of Hg poor in water. When we take a liquid rich in water, the 
reaction is: 

L2k+k’+4. AV,>0. 
4th AG 
RP’ tL +G4 PAR +G. 
Retr’ E 

As the reaction proceeds from left to right with increase of volume 
(AV, >0), the equilibrium to the right of the vertical line occurs 
on decrease of pressure and the equilibria to the left of the vertical 
line oceur on increase of pressure. Therefore, from each point of 
branch pQ the equilibria /”-+ 1+ G and I'"+ L + G proceed 
towards higher pressures; consequently we find the rule 1¢. 

When we take a liquid poor in water, this is situated on /ZS or 
on Sq. When it is situated on /7S, the above-mentioned reaction 
applies also, but OV, <0. Therefore, from each point of branch 
HS the equilibria #’ + 1+ G and #'" + L + G@ proceed towards 
lower pressures; this is in accordance with rule 1%. 

When we take a solution of branch Sg, the reaction is: 

+ FY’ S Lt G. AV, >0. 
M+R A LE Iv tL+G 
MAR’ AG | FP+AL+G 

As the reaction proceeds from left to right with increase of volume 
the equilibria to the right of the line oceur with increase of volume. 

In accordance with rule 1° we find, therefore, that the equilibria 
FtL+G and F"4+ L4G proceed from each point of the 
branch Sq towards lower pressures. 

Now we have deduced the rules 1¢ and 1? assuming that point #7 
is situated on branch pS; we may act in a similar way when point 
H is situated on branch gS. In a similar way we can also deduce 
the rules 2 and 3. 


85 


Considering, instead of the saturationcurves the boiling point 
curves, the same applies to these in general. We must then replace 
on the fourphase-curve the point of maximumtemperature by the 
point of maximum pressure. In fig. 3 besides the point of maximum- 
temperature H, also the point of maximum-pressure Q is drawn. 
We imagine further that the saturationcurves are repiaced in the 
diagrams by boilingpointeurves. We then refind the rules 1, 2, and 
3, with this difference, however, that increase of pressure must be 
replaced by decrease of the boilingpoint and decrease of pressure by 
increase of the boilingpoint. 

From each point of the four-phase curve proceed two saturation- 
curves and two boilingpointecurves. When this solution is to be 
considered as rich in water or as poor in water with respect to the 
saturationcurves, it is also the same with respect to the boiling- 
pointeurves. Only the solutions between the point of maximum- 
pressure and the point of maximumtemperature make an exception ; 
these are rich in water when we consider the saturationcurves, 
poor in water when we consider the boilingpointcurves. Now we 
find: from a solution saturated with two solid substances the vapour- 
pressure (along one of the saturationecurves) and the boilingpoint 
(along the corresponding boilingpointcurve) change generally in 
opposite direction. When, however, this solution is situated between 
the point of maximumpressure and the point of maximumtemperature, 
vapourpressure and boilingpoint change in the same direction. 


(To be continued). 


Physics. — “On the thermodynamic potential as a kinetic quantity”. 
(First part), By Dr. H. Hunsnor. (Communicated by Prof. 
J. D. VAN DER WAALS). 


(Communicated in the meeting of April 24, 1914). 


In a communication published in These Proc. Il p. 889 of Jan. 
27 1900°) it has been set forth by me that in the capillary layer 
the molecular pressure must have a different value in different 
directions as a direct consequence of the attraction of the particles, 
whereas the thermic pressure (the sum of the molecular and the 


1) I expressly call attention to this date, because some time after, this subject 
was treated in the same way by a writer who had informed me of his own 
accord that he was going to publish an article on this subject in the Zeitschrift 
fiir phys. Chemie, and that he should of course, cite my paper there, but who 
has failed to do so. 


86 


internal pressure) must be the same in all directions. Hence a 
condition oceurs in the capillary layer in which the external pressure 
in the direction of this layer p, has a quite different value from the 
pressure normal to this layer p, i.e. the pressure in the homogeneous 
vapour and liquid phases. In the surface a tension appeared to exist: 


fo. —p,)dh. 


The molecular pressure could be easily defined so that the surface 
tension was in agreement with the capillary energy determined by 
Prof. vAN per Waats by a thermodynamic way : 


fee —T,y + p,w—pM)dh, 


1 : : : 
in which ge—=— and v is the volume for a molecular quantity of 
v 


MW grams and 


c, d*o Cy d‘o 
2d 4) dh” 

The two integrals, which must be extended over the full height 
of the transition layer, are equal, and this is also the case with two 


p= (6) ao 


corresponding elements so that: 
o(e—T\y + p\v—uM) = p,— Pp, 
from which immediately follows 
e—T7 yn 4+ pv=ul. * 

As p,, the pressure in the direction of the capillary layer, has 
the same value in the homogeneous vapour and liquid phases as 
p,, it holds for the quantity 

e— TI, + pyv 
that i has a constant value both in the homogeneous vapour and 
liquid phase and in the capillary layer. This property leads us at 
once to expect that if will play an important part especially for 
kinetic considerations, and that it will express that the number of 
particles that two arbitrary phases will exchange in the same time, 
will be equally great. It will, in fact appear that this quantity 
makes the capillary layer accessible for the considerations developed 
by Prof. vax per Waats in his paper on the kinetic significance of 
the thermodynamical potential. Assuming that really in the direction 
of the capillary layer the pressure p, is different from the pressure 
p,, and besides entirely different in different layers, the neglect of 
this circumstance will make it impossible to derive the thermodynamic 
conditions of equilibrium for the capillary. layer from kinetic con- 


87 


siderations. A particle, namely, that begins a new path at some 
place, is subjected to the influence of the pressure p, prevailing 
there, and in the layer, where it terminates this path, it is subjected 
to the in general entirely different pressure p, of this layer. 

Van per Waals’ first equation runs: 


a a 
dmNu,? + pr, — — = 4mNu',? + pu» ——-. - . . (1) 
v v 


1 2 


The expression pv, — - = G = ) is for a monatomic fluid the 
2 1 
heat of evaporation for the molecular weight, «, -+ pr, —(#, + pr,). 
We shall now have to apply a modification to this equation, when 
the layers between which the interchange of particles takes place, 
are taken in the capillary layer. Here we shall have, as it were, 
an evaporation from a space under the pressure p, towards a space 
under the pressure p’,, and a condensation in opposed direction. 


Hence our first equation becomes : = 
ImNu,,? aL Cs d*9 1 Nu! an teat ' Cy d*o! 1) 
<miNU p,v—ao — — — == 5mLlVu ?,v —ago — — — - 

2 n Ps N 2 dh? n Ps N 9 dh? ( 


The equation which expresses that for a stationary state a group 
of particles from one layer will be replaced by a group of particles 
from the other layer becomes just as vaN DER WAALS puts: 


ane Wn 
1 e j 1 a i 
€ tin, =——— 6 w', du'y 
v—b 0 
Now from (1) follows : 
Un Uy 1, AU a 


and our second relation becomes therefore : 


Un? Dee 
1 a 1 ae ‘ 
v—b : Ta p25 z (4) 
hence : 
ay Hs d*o' c, d’o 
ae ee pv —ay'— ~ |—| p,v—ag— = 
i v—b ImNu,?—tmNu,? 2 dh? 3 2 dh? 
0 = + ___ — + 
ae tmNa? MRT 
or 
c, 0 a cad: oO i ae 
ag-— —~-MRTlog(v-b) + p,v = -ao0'-— —~-MRT log(v'—b) + pv = Mu (3) 
2 dh? ‘ ™ i 2dht ; y ; 


88 


e— Ty + pe Se — Pig pe Mae 


The validity of the relations (2) and (3) may be established by 
means of BoLtZMaNn’s equation modified by van Der WaAats 


M |(Xdx + Ydy +Zdz) 


nS MRT ’ 
in which M | (Xde + Ydy + Zdz) represents the work done on the 


be 
molecular quantity on transition from a layer with density — to a 
Vv 


layer with density —. 
in 
When in a point of the capillary layer at h the energy with 
omission of the constant amounts to 
c,d°o ¢, d‘o 
=== 00) 
2 dh? 4! dh’ 
the molecular pressure in this point in the direction of the layer 
Cems om Or  eh10) 


4 
a 1 he Ty ay Saga 


20 


As 


can be represented by — ee = ag? + 


Vo 
ag? + So. ; (enz.) =p + ag’, 


in which p represents the pressure belonging to the homogeneous 
phase of the density 9, we have 


‘ 
c, do 


aaa: 
PPG OF 


If we substitute p, from this relation in (3), the latter passes into : 


1D = 1 = 


do 
— av —¢, Te MRT? log (v — b) + puo=ul. 
ah 


This equation, which we have derived by the aid of kinetie con- 
siderations, is the condition of equilibrium, at which Prof. vAN DmR 
Waats arrives in his ‘“Thermodynamical theory of capillarity” 

Following in Prof. van per Waaus’s steps, Dr. A. vAN ELprk has 
given a thermodynamie theory of the capillarity for a mixture of two 
substances. By applying that the total free energy must be a minimum 


> 


for all variations of @ and a, which satisty fg dh = constant and 


fe (1 — x) dh = constant, he found for the variation with respect to @ 


89 


f(ex)+o af —— a, M, (1-«) — uw, Mx — ¢,, (1-«) diet ae) c, (1-2) Gee — 
INS ry do ess M243 11 dh? 13 dh? 
d’o(1-«) Pou 
eer emi” 75 eee 


In this f(@z) is the free energy of a homogeneous phase with 
the w and o existing in /, and hence 


— MRT log (v—b,z) — ae 4+- MRT \(1—2z) log (1—«) + «@ log 2}. 
t . t v ‘ s 


of 
o an = pv 
The energy for M, grams of the first ee amounts to 
eh dc. (1—2) M.. dow 
é, = C,—a,, 9 (l—2) —4,, 9@ — 3 ¢, un Fe ie a 


and for J/, grams of the second component : 
% d°o(1—-2) d* ow 
&, = C, — a,,0(1—2) —a,, 0 e — $.¢,, ——>—__ — 36 2 


dh* anes dh? 


We get therefore for our equations (1) for the first component : 


me. ELAN a A ig d* o(l—a ) dou 
1m,Nu, ? + ——— — a,,90(1l—e# ox — te -—1¢, —_= 
et it o (1-2) 118 113 Le dit 219° apa 
tm, Nul, 2+ se Be Nie ni ay nme Ea OS Ney 
tan Ni. a @ )—a,,.9 & —3C; Sam 2 iis =e 
as AGE ian Bi eae ge dh? ; 
and for the other component: 
d’o(1-w) doa 
$m, Nu, Le SEO —z)—a, 29 — SACts aang <a aa 2 
Ut dh dh 
' a 2 ! 
4 d’o'(1-«’) o'r 
© 2 2 
= 2m Nu’, ; = = 4150 0 (1-é t')—4,,0.0 — b Cis — qo)! $ Cy5— = 3 (1,) 
ou dh dh 


In this a represents the partial pressure so that in the homogeneous 
phase ,a is the partial pressure for the first component, and ,a the 
partial pressure for the second component. ,2 + ,.7 =p. In_ the 
direction of the capillary layer these partial pressures are represented 
Dye dean 2K... sO: that oa, a. — 

a Ea) 
mm ao 2 1 2 . # a 
thes expressions ——_—_ (Or —, therefore, represents the work done 
o(1—~) l—a 
on a quantity J/, of grams of the first component when it leaves the 
phase. The phase being composed of J/, (1—a) +-J/,v grams in a volume 
. . . v 
M, grams of the first component will occupy a volume 


al 


90 


The equations (2) which express that for each of the components 
a group of particles from one phase is replaced by a. group of 
particles from another phase, become for the first component: 


1 Ju. 2 nt 7; 2 
tm, a din, Nu 1, 
hey cay TAT ESS 1p M ee Way 
Sse ty dts 3m, C= ie Git. weve aU Grae (2,) 
! 1 1 1 
v—by. n a v — by n n 
and for the second component: : 
1 Ty. 3 1 lea 
tm, N tls tm, Nu’, 
A aa Bal ogo ; ee nue 
wv i, ipa av it 2 
—u, du, e 3m,Na,* —_" —u', dui, e pm, Na,” 3 ((2,)) 
y—D n n — by n n 


Taking into consideration that 2, dea, = wu, ds, and us, dua, = 
= u's, du's,, and that 4m, Na,?=4m, Na,?= MRT, we may write 
for (2,) and (2,); 

7. 2 1 leis. x] 
pe, Alcs bm, Nu, | — km, Nu ty 
log ame = Ul = a Vy Ty 
i= 05) he MRI 
and * 


j= Bee bm, Nu, > — Im, Nu', * 

re n 

log ae es ee 
yb, of “URI 


from which then follows for the first Component in connection with 
Ge) sama yar) 


pe =n) note d*o(1-«) 
\T log =e +- 65) —4,,9 (1-2) -a,,0%-}¢,, 7 
d* ow Ore Roce ; : Per } 
— 3Cr, dh? — MRP log jaa AG o'(1-a") wane (1-a')-a,,g'@ ik (3,) 
?9'(1-z') d?9'x' a v 
— 3¢, dit aga Gays =e, — Tn, eg 
and for the een component : 
P 1? o(1-« \ 
— MRT log - Sow 242 a 4129 »(1-«) —a,, ow —3e paul ae 
x ox dh? 
dow Fa eS OE Pate a ; 
—4¢,,—,,— — MRT log—__ + = 40 1-0) — oh 0 
dh a Ou 
d?o'(1-2') d?o'a' v 
21g dhe San Cas dh? 5 Ty, + 5% 2a =o uM, . 


The expressions : 


2 


Vv 
é, — Ty, + 17, ae and é 


LU 


v 
— Ty, + .2, —=u,Y, 
& 


have a constant value throughout the vessel. For every component 
they give us the thermodynamic potential in its kinetical signification. 


91 


When we now write the value of w.J/,(1—.«)+ yu, Je, we tind 
for it, at the height of / with density y and concentration « 
— MRT SU rsdeiag MRT \(1 = x) log (1L—w) + wx log x} +- pv — azo — 


d*o0(1-«) ; dou ; d*o(1 x) 
= $og(1—2) ell a Ge 2 Oy gt ii 
ad’ ox 
ba VU, (l-«) +m «; 
for 
iT, ay 
== —— 0 
Q Q 


The pressure p, can be expelled from this relation when we 
consider that p;-+ 4, (molecular pressure in the direction of the 


capillary layer) =p--a.e*, in which p represents the pressure 
belonging to an homogeneous phase of the same density and con- 
centration. In general M, = — 0 fe, — C, (A-—a) — Cyz} holds, in 


which ¢ = ¢, (1—w) + ¢,7, hence the energy for the quantity of the 
mixture M, —2) + M,x. Now: 


4 d’o(1—z) 
&; = C, (l—a) + C,z — a9 — }¢,, (1-—«) 


dh? 
age +, d?9(1—-x) Pow 


are) dh? Ne dh? — $450 dh? 
hence 
; Eola, do. SOE) dow 
i= $C, (1-2) dh? ¥ 4c,,(1- x) — dh? mat} 2 Oya? Ae 5p Qt dh? 


If this value of p, is introduced, the found relation passes into 
— MRT log (v —b,) + MRT \(1 —«) log (1—a) + «log x} + pv — arg — 
d° oe 2) d? ow d*o(1-«) Pox 
— ¢, (I-2) 72 —¢,, (1-2) dhe ks a dhe meas ae = 
= uw, (1—2) + u,M,« 


This relation, which we have derived by means of kinetic consider- 


ations only, is the first of the two conditions for the equilibrium 
determined by van Expik by a thermodynamic way. 

For the two homogeneous phases, which are in equilibrium with 
each other, the following form holds: 
—MRTlog(v-b,) + MRT}\(1—a)log(1-«) +- wloge} + pv-a,o=, VM, (1-2) +4, Mya 
or 

yw -}+ pv = "MY, (l1—2) + uM. 

As the kinetie theory teaches that the pressure in the two phases 

must be constant, it follows immediately from this that: 
yw — J, (1—2) — vw, Ma 


— Pr . 


v 


9? 


Chemistry. — “On the behaviour of gels towards liquids and the 
vapours thereof.’ Il. By Dr. L. K. Wore and Dr. E. H. 


Bicuner. (Communicated by Prof. A. F. Honieman). 


(Communicated in the meeting of April 24, 1914). 


In continuing the experiments mentioned in our first communi- 
cation about this subject"), we hit upon two observations which 
have given us the key to the solution of the problem. Firstly it 
was found that, when leading saturated water vapour over gelatine 
which at the same temperature had swollen in water, the weight 
of the gelatine does not change; secondly it appeared that the 
amount of decrease with the experiments made in the previously 
described way — in desiceators according to VAN BreMMELEN — 
depended upon the size of the desiccator, and besides that in this 
way of experimenting pure water also lost in weight. These things 
found, we came to the following conception of von ScHROEDER’Ss 
phenomenon : 

1. the state attained in water vapour is no equilibrium ; even 
though the quantity of water absorbed does not visibly increase for 
days and days, one must suppose an extremely slow absorption still 
to be taking place, at least if the experiment is made in the exact 
way which will be presently deseribed. However, it may be several 
years, before the true equilibrium is reached, which in liquid water 
appears within some days. So the so called vapourequilibrium is 
only a ‘false equilibrium”. 

2. the curve which indicates the connection between the water 
content and the vapourtension, runs almost horizontally as soon as 
the point which represents the vapour equilibrium, is passed; the 
tension being taken as ordinate, the concentration as abscissa. 

3. The observation formerly advanced by von ScHroepmur, BANCROFT, 
and also by us against the hypothesis mentioned under 1, viz. that. 
the watercontent of gelatine swollen in the liquid. decreased again 
in vapour, (from which was concluded that the ‘equilibrium’ was 
attained from two sides), is founded on an unsatisfactory way of 
experimenting. This conception seems to give a satisfactory explana- 
tion of the whole of the phenomena; we can support it by a great 
number of experiments. 

We shall now first of all treat the proof of the third thesis. As 


1) These Proce. 15, 1078 (1912/18). 


93 
we doubted about the exactness of the method with desiceators, we 
made experiments in another way. We let a piece of gelatine swell 
under water until the equilibrium was attained, put it into a U- 
tube with ground stopeocks, hung this tube in a thermostat, and 
sucked a stream of air saturated with watervapour through it. In 
order to fully saturate the air with watervapour, we let it pass 
in extremely tine bubbles through four tubes of water which were 
also hanging in the thermostat. We made sure of the vapour really 
being saturated by placing a U-tube filled with water before the 
U-tube with gelatine, and by also weighing the former before and 
after the air had been led through. 


Nasi Is ke 
Time Weight of U-tube Weight of U-tube 

++ water + gelatine 

| 30.130 | 30.779 | 
24 hours | 30.127 30.781 | Temp. 19°.0 
267". | 30.126 | 30.779 | (in thermostat) 
[Sin | 30.123 30.778 
Hts wy tl 30.117 | 30.780 


It will be seen, that the gelatine, coutrary to our former experi- 
ments, showed no decrease of weight: if was in equilibrium and it 
remained so, and there was not the slightest abnormality. Now 
which method, the old or the new one, is more reliable ? The 
answer cannot be dubious, for we succeeded in improving the old 
method to such an extent that if gives the same results as the 
new one. 

Formerly we used to place little dishes of gelatine in a ScHErBl.Er- 
desiccator, at the bottom of which was some water, and which 
stood in a room of a fairly constant temperature. In order to exclude 
the possibility that the water from the gelatine, under the influence 
of gravity, should distill to the water at the bottom, we have now, 
instead of pouring the water into the desiccator, placed a dish of 
water at the same level as that with gelatine. And, thinking of 
Foorr’s experiments mentioned in our first communication, we also 
weighed this dish, expecting, of course, that the water lost by th 
gelatine, should be found back here. However it appeared that 
both gelatine and water equally decreased in weight; (it is to be 
noticed that the desiccator was not evacuated). 


94 


DAB GE MI: 
Tt a Weight of dish ranean’ Weight of dish 
Time aaatar decrease + gelatine decrease 
47.458 48.391 temp. 22° 
(room). 

24 hours 47.238 .220 48.209 . 182 
24k 47.031 207 48.009 . 200 
Bs 45.868 163 47.863 . 146 
a || 46.5067 | .301 47.525 -338 


2nd experiment (three dishes of water). 


a 
time weightn9l decrease weight n°2 decrease weight n°3 decrease 

| | 

| 


81.129 | | 64.399 | 45.888 | temp. 22° 


| | | (room). 
24 hours 80.868 | 261 64.041 scien | heel eat 


94 80.601 | 267 63.709 .332 45.291 | .300 


We see from this that, in taking the experiment in this way, a 
dish of water decreases in weight 200 to 800 mG. in 24 hours, and 
that consequently the experiments thus made with gelatine, do not 
prove anything whatever. 

It is not quite easy to say where this water goes to. It might be 
thought that if serves to saturate the whole space of the desiccator 
with vapour; but for this a much smaller quantity suffices, 1 L. 
saturated watervapour of 22° only weighing 19 mG. Nor are 
differences of temperature probable, because the changes we have 
found always go in one direction, and because we cannot think 
why the water in the middle of the desiceator should always be 
warmer than the walls thereof. Besides the temperature in the room 
was rather high'), only varying within 0,5°, and so the dishes, 
after being weighed, would sooner enter colder than warmer. 
It was also controlled if a loss of weight occurred during the 
weighing and the preparations for it; by working quickly however, 
this loss could easily be kept under 1 mG. The only explanations 
left are, either the watervapour diffuses to the outside, passing 
through the layer of grease which is between the desiccator and 
the lid, or water is adsorbed at the great glass surface of the de- 
siccator. The latter explanation will be most probable, as in smaller 


1) Except in two series of table IN), where the differences are equally great 
all the same. 


95 


IpAy Bybee eit: 


Small desiccator of FRESENIUS; temp. room 22°. 


: weight dish 1 |... weight dish2 | 4.00. 
Time -P water decrease - water decrease 
| | 
33.798 21.409 
| 
48 hours) 33.745 053 21.382 | 0.027 Volume of the 
48, 33.722 023 21.360 | .022 | desiccator: 700 c.c. 
dish 3 | dish 4 | 
+ gelatine -++ water | 
| 
31.584 27.566 
24 hours) 31.573 O11 27.545 021 
240s 31.561 012 27.527 O18 | 
24) 4 B1549 eer O12 27.510 O17 
120 , 31.505 044 | 27.471 039 
water water | 
——+ ae ee 
31.621 27.834 
24hours 31.605 016 27.819 O15 
temp. room 14° 
24 31.585 020 27.800 | .019 
AN 31.565 020 Ditties e023 
pee Ae Se i oa 
gelatine | | 
27.764 | Qe | 
72hours|) 27.741 .023 | 27.7159 018 temp. room 16°.5 
48, 27.724 O17 27.739 .020 | 
Bell-jar in pail; temp. room 22°, 
EEE 
weight of weight of 
Time weighing-bottle decrease Time  weighing-bottle decrease 
+ gelatine -+- water 
36.116 40.407 
90 hours: 36.052 .064 5 hours 40.411 (-+.004) 
SOL. anal 36.026 026 48 , 40.250 161 
18 | O17 Poth ge 40.122 . 128 


» 36.009 


Yb 


desiceators — model Fresenius — we found much smaller decreases, 
and as we also found a loss of weight when making the experiment 
differently. A glass bell-jar, in which was hanging a weighing-bottle 
with gelatine swollen in water, was partly placed ina pail of water, 
so that the gelatine remained some em. above the water surface. 
There can here be no question of diffusion to the outside. Yet the 
adsorption hypothesis is not without its difficulties; for in taking the 
above mentioned experiments the desiccator or the belljar were first 
well rinsed out and moistened with water, so that one should think 
the glass surface to be entirely covered with a layer of water. 
Perhaps the two last mentioned causes of decrease of weight are 
cooperating. 

Whatever may be the cause of decrease, we can distinctly see by this 
able that both water and swollen gelatine decrease. So if we wished 
to really confirm voN ScHroEDER’s observation, we first ought to have 
an arrangement with which water only does not diminish in weight. 

A series of experiments, undertaken in consequence of Foorr’s 
communieation which has been mentioned before several times, will 
illustrate how hard it is to make exact observations by the statical 
method. In a glass tube were two small tubes filled with water 
above one another, which had been weighed before. The tube was 
closed with a rubberstopper or it was sealed in the flame, and then 
placed in a thermostat; after two days the tube was opened, and 
the little tubes were quickly put in weighing bottles, and were 


weighed. 


PAS Bees EMV: 
| | “an 
himey ete lowet ‘decrease | Welg BtUBper | decrease 
| 22.098 24.000 
48 hours 22.090 | -008 | 23.992 | 008 temp. 18°.0 
48, 22.081 009 | 23.980 | .012 rubberstopper 
ond experiment. | 
22.060 23.923 
48, | 22.051 |  .009 | 23.918 | .005 | id. id. 
3rd experiment. 
10.108 | | 36.289 | | 


AB 10.098 010 36.244 045 | sealed 


of 


So we again found a decrease of weight in all cases, be it less 
than with the experiments made before. As the amounts are so much 
smaller here, another circumstance, except the one of adsorption at 
the glass walls, must be taken into consideration, which, as we have 
found with the apparatus presently to be described, can account for 
differences to an amount of some mG.!) The tubes were opened 
outside the thermostat; the outer’ walls then cooled down a few 
degrees, while the inner tubes remained a litthke warmer. In those 
few moments a small quantity of water could distill to the wall of 
the great tube, and this may be the cause of the loss of weight. 

Now in order to exelude adsorption we have passed on to another 
arrangement. We had a cylindrical box made of brass (measures: 
diameter 7.5 em., height 7.5 em., volume 320 ¢.c.), which was 
closed by an exactly fitting brass lid that could be still more strongly 
fixed on by screws. Both the box and the lid were silvered at. the 
inside. The apparatus was entirely plunged into a thermostat, kept 
constant within O°.1. In this apparatus too we began with weighing- 
bottles, which only contained water; we again had to state a loss 
of weight. With these experiments the vessel was taken out of the 
thermostat, and was quickly unscrewed after which the weighine- 
bottles were taken out and weighed with their stoppers closed. 
When a closed weighing-bottle with water was placed in the vessel, 
the weight remained constant; when taking if out, some sheht 
moisture was to be seen against the stopper. A refrigeration evidently 
took place here, by a colder stream of air entering when the lid 
was taken off. In order to avoid this as much as possible, we placed 
the apparatus rather high in the thermostat; when it had to be 
opened we made the water run out of the thermostat through a 
siphon, so far that the lid appeared just above the watersurface. 
Meanwhile the screws were unscrewed so that the lid could be 
taken off as soon as it was above the waterlevel; in this way the 
whole kept the same temperature until the very last moment. The 
then obtained results were satisfactory (ep. table V), and we there- 
fore repeated our experiments with gelatine-water, agar-water, and 
celloidin-aleohol in this way. 

From these experiments we learn that gelatine, agar, and celloidin 
swollen in a liquid, do not undergo a loss of weight when placed 
in saturated vapour, if the experiment is made rigorously. The results 
with the celloidin-aleohol system are not so good as with the others, 
it is true, but the decrease which reached an amount of 1O0—200 

') The greater difference in the upper tube of the 5rd experiment is evidently 
due to the heating during the sealing process. 


Proceedings Royal Acad. Amsterdam. Vol. XVII 


98 


TAY BLEW. 
Temperature 19°.0; weighings every 24 hours. 
weight of weighing- |... | weight of weighing- 
bottle 1 -+- water decreas] bottle 2-+- water decreas 
26.045 25.096 
Ist series 
water | 26.033 .012 25.088 008 
vessel opened 
outside the 26.025 008 25.081 007 
thermostat | 
26.012 013 25.069 .012 
2nd series ; 2 
rarer 25.772 27.837 
vessel opened c ; 97 @ 
in the thermostat 25-1168 004 ay Eos 003 
| weighing- bottle | 
+ gelatine 
20.136 The gelatine had been 
90:13 wa swelling for a fortnight in 
Beit exaas Wess) ; | water at a temperature of 
Pate ae 20.135 0 19°.0, and had been dried 
gelatine with filter paper before the 
| 20.135 | 0 experiment. 
| 20.133 -002 (after 3>< 24 hours). 
| | | 
Temperature 21°.4. 
24.575 | 
Mls arine Da AN | The agar had been swel- 
ALN | BOE | (+ -005) | ting for 8 days under water 
agar 24.582 | (+ .002) | at the same temperature, and 
had been dried as said above. 
| 24.581 | .001 | 
Temperature 21°.4 
3 SEEEREEeaeiemeed 
NO, | NO, 2 No. 3 N°. 4 
| | | | 
| | | | | 
12.202 12.122 | | 12.389 | 11.310 | 
5th series | | | | after 
celloidin- | 12.200 | .002 | 12.108 | .014 | 12.379 010 304 | .006 | 42 hours 
alcohol 
12.095 | .013 | 12.370 Ne | 11.301 | AGO || ES 
Temperature 0°, 
| 12.248 12.115 | 12.397 | | 
| I | | 
6th series) 12.255 | (+.007) | 12.113 | .002 | 12.399 | (+.002) | after 61 hours 
celloidin | 12.249 .006 | 12.109 | .004 | 12.396 20033] ins & 
| | 
12.249 | 0 0 12.395 | S001) 24 > 


12.109 | 


| { 


99 


mG. with the old method, has been reduced to some mG. only ; 
we must herewith remember that the vapour tension of alcohol is 
considerably greater than that of water. Therefore the 6" series of 
experiments was undertaken at 0°; according to our expectations the 
results were better than at 21.4°. 

The experiments communicated here have taken away every actual 
ground of existence from the opinion expressed first by von ScHRoEDER, 
viz. that here was a conflict with the second law of thermodynamies; 
the second law, as one might think, remains untouched. Of course 
the phenomenon of several substances swelling more in liquids than 
in vapours, remains; but we think this can be sufficiently explained 
by assuming that the absorption in vapour occurs extremely slowly 
in the end. We have also investigated if not totally swollen geiatine 
and celloidin placed in vapour, would absorb more water in our 
new apparatus, and would come to the real equilibrium. This 
appeared not to be the case; e.g. with gelatine of the following 
compositions: 1 gelatine to 26 parts of water (in weight); 1:24,2; 
1:18,8; 1:15,8; 1:6,5, (the ‘false vapourequilibrium’” is about 
1: 0.7) no change of weight was found for five days’). So it goes 
without saying that the absorption takes place exceedingly slowly. 

This is most probably connected with the fact that the vapour 
tension of gelatine (and numerous other substances) is already very 
near to that of pure water when they have only absorbed a rather 
small quantity of water*); consequently all the further water absorp- 
tion of any importance is only of slight inflaenee upon the vapour 
tension. Or in other terms, the difference of the vapourtension of 
pure water and of gelatine in “vapourequilibrium” is very small, 
and consequently the absorption velocity will also be very small. 
That it is yet very great in liquid water, may be easily explained 
from the density which is 50000 times greater. 

We just wish to state that the determinations meant here have 
ail been obtained by the statical method, the deficiency of which 
we have proved; a true opinion can only be possible if the experiments 
are taken along the dynamical way‘), and if the real equilibrium 
has been proved by placing the jellies alternately in vapour of 
higher and lower tension. The values given for the composition of 
the substances swollen in the vapour of pure water are never true 


‘') These experiments were also made in the dynamical method with U-tubes, 
yielding the same result. 
») Katz, these Proc. 18, 958 (1910/11). 


5) Or m the apparatus described above. 


100 


equilibria; one ought to state the value which is attained in liquid 
water °). 

The explanation of the phenomenon becomes somewhat different, 
if we do not let the gelatine (ecelloidin) swell in pure water (alcohol) 
but in solutions. In case of the dissolved substance being volatile 
(example: celloidin-aleohol-water), the circumstances are exactly the 
same as above mentioned; but, if the substance is e.g. a salt, the 
thing changes. Von Scurogper has made some experiments about 
this question, and he ascertains that '/,,,,,,-"norm. sulphate solution 
already lowers the vapourtension of gelatine so much, that there is 
not even a decrease in vapour, but an increase. After the results 
deseribed above, voN ScurorpEr’s argument loses all weight, and 
his result is sure to be due to chance. . 

It is a fact we have repeatedly observed, that gelatine (celloidin) 
which had swollen in the vapour of a salt solution (NaCl in water, 
resp. HeCl, in alcohol) absorbs much more still, when brought ito 
the liquid; 1 Gr. celloidin e.g. gains 1,77 Gr. in weight in a solution 
of 4°/, sublimate in alcohol of 96°/,, whereas only 0.89 Gr. is 
absorbed in the vapour of aleohol, and consequently still less in 
the vapour of a solution in alcohol. The difference between the 
swelling in a pure liquid and in a solution finds its cause in a 
substance, when in the vapour of a solution, never being able to absorb 
anything but the solvent, as long as the dissolved substance is not volatile; 
when placed in the liquid itself, it also absorbs the dissolved substance. 

This is a wellknown fact about gelatine; we have ascertained 
by the experiments with celloidin mentioned above, that this substance 
too had not only absorbed alcohol, but also sublimate. So in these 
cases it is clear for other reasons, that a substance swollen in vapour, 
when brought into the liquid) phase, must still absorb more, and 
that the state attained in vapour is not a true equilibrium’). In 
vapour e.g. celloidin passes into celloidin + alcohol, until the vapour- 
tension of this phase has become equal to that of the liquid phase: 
alcohol + HgCl,. Now if one brings the celloidin phase under the 
liquid, the HgCl, diffuses into the celloidin; diminishes so to say 
the vapourtension of the alcohol which is contained therein, and 
consequently a furtber absorption of alcohol must take place. If we 


1) Strictly speaking one must not speak of pure water, but of a saturated solution 
of gelatine, agar ete. in water; of course, the difference really is exceedingly minute. 

2) Cf. Totman’s views, J. Amer. Chem. Soc. 35, 307 (1913). We have 
assumed with ToLMAN that every substance evaporates somewhat, no matter how 
little; if one objects to this, one must speak of an equilibrium which lies differently 
in consequence of passive resistances (GIBBS). 


101 


represent this by a figure, we obtain in the vapour a state @; and 
after this the state 6 is reached in the liquid along an exactly 
horizontal line, for the vapourtension remains absolutely the same ; 
only the composition of the celloidin changes. @ lies of course at 
a lower pressure than «@ in the figure, which stands for pure 
alcohol; in the latter ab’ is only approximately horizontal. 


iE : oy b 


2 XK 


It is evident that in this case the greater absorption in the liquid 
must be connected with the solubility of the salt in the gelatine or 
celloidin. According to the colloid absorbing more salt, the difference 
between the vapour and the liquid equilibrium will be all the greater. 
We believe a closer study of this subject may probably bear fruit 
with a view to the knowledge of the behaviour of jellies in different 
solutions. We intend to start experiments about this with celloidin, 
which, as to stability, has great advantages over gelatine with which 
suchlike experiments have been made up to the present’). We do 
not consider skinpowder an ideal substance for this purpose either *). 


As a summary we think, we can say that the pretended conflict 
with the second law of thermodynamics has been put an end to, 
and that von Scurogper’s phenomenon in the principal case is due 
to a slowly coming equilibrium; one may expect it in all cases 
where the vapourtension already approaches the tension of the pure 
liquid very nearly, a long time before the equilibrium has been 
attained. If the liquid absorbed is a solution of a nonvolatile sub- 
stance, another explanation must be given. 


Path. Anat. and Inorg. Chem. Lab. 


University of Amsterdam. 
1) HormeEIsTER, among others. 
*) Herzog and Apuor, Koll. Zeitschr. 2, Supplem. heft 2, (1908). 


102 


Mathematics. -- “The quidruple involution of the cotangential 


points ef a cubic pencil.” By Professor Jan pe Vries. 
(Communicated in the meeting of April 24, 1914). 


1. We consider a pencil of cubies (v*), with the nine base-points 
4,. On the curve gv’, passing through an arbitrary point P, lie three 
points P’,P",P", which have the tangential point’) in common with 
P; in this way the points of the plane may be arranged in qua- 
druples of an involution (P) of cotangential points. We shall suppose, 
that the pencil is general, consequently contains fivelve eurves with 
a node D,;. On such a curve dé all the groups of the (P*) consist 
of two cotangential points and the point D, which must be counted 
twice. Apparently the 12 points ) are the only coincidences of the 
involution; as the connector of the neighbouring points of D is quite 
indetinite, the coincidences have no detinite support. The points Dy 
are at the same time to be considered as singular points ; to each 
of them an involution of pairs P,P’ is associated, lying on the curve 
J),*, which has D, as node. 


2. The nine base-points Br are also singular; to each point Lb, 
a triple involution of points 2”, P", P" is associated, lying on a 
curve B,, of which we are going to determine the order. 

To each curve g* we associate the line 6, which touches it in B; 
in consequence of which a projectivity arises between the pencil of 
rays (b) and the eubie pencil (*). The curve tr produced is the 
locus of the tangential points of B (tangential curve of B). 

The line 6, which touches a g* in £#, cuts it moreover in the 
tangential point of B; this is apparently the only point that 6 has 
in common with +r’ apart from B. So rt! has a triple point in By 
there ave three lines 6, which have in # three points in common with 
the corresponding curve g*; i.e. B is point of inflection of three 
curves g* 

Let us now consider the tangential curves rt‘, and t*,, belonging 
to b 


consequently have apart from the peints 4, three points in common ; 


, and #,. Both pass through the remaining seven base-points, 
so there are three curves g*, on which B, and 4, have the same 
tangential point. Hence it ensues that the singular curve 3, belonging 
io B,, has triple points in each of the remaining eight points Bb; 
it does not pass through 2B, because (/') has coincidences in D, 


1) The ¢angential point of P is the intersection of 9% with the straight line 
touching it in P. 


L038 


only. With an arbitrary g*, 3, has moreover in common the three 
points which form a quadruple with 4, ; consequently 27 points in 
all. So the triplets of (P') belonging to 4, lie on a curve of order 
nine, Which passes three times through each of the remaining base-points. 

We found that 5, and 4, belong to three quadruples; the three 
pairs, which those quadruples contain besides, belong to the singular 
curves 3,’ and ~#,°. They have moreover in the seven remaining 
points 5;, 63 points in common; the remaining 12 common points 
are found in the singular points Dy. 


3. The locus of the points of inflection / of (~*) has triple points 
in Br, has therefore with an arbitrary v*, 9 x 3+ 9 = 36 points 
in common; it is consequently a curve of order twelve, v?. On a 
curve d* lie only 3 points of inflection ; we conclude from this, that 
v= has nodes in the twelve points DY, ; in each of those points «4 
and d* have the same tangents. 

The points P’, P', P'", which have / as tangential point, lie in a 
straight line, the harmonic polar line h of I. So e* is the locus of 
the points, which in (77) are associated to dinear triplets. 

The curves p,° and <«* have in the singular poiits LB and D 
8 x 37-12 x 2=96 points in common; on @,’ lie therefore 12 
points 7, so that B, belongs to 12 linear triplets. From this it ensues 
by the way, that the involution (/*) lying on p,° has a curve of 
involution (p) of class twelve; tor the line p= P’P" will only pass ~ 
through B, if P" is a point of inflection, while P lies in 4,. As 
B, is point of inflection of three g*, (P*) has three linear triplets, 
consequently (p),, three triple tangents. 

The locus 2 of the linear triplets has, as was shown, 9 dodecuple 
points B; as g* bears nine points of inflection, therefore 9 linear 
triplets, it has with 4 9 >¢ 12-49 < 38=1385 points in common. 

Consequently the linear triplets lie on a curve 2". 


4. We shall now consider the curve g, into which a straight 
line ¢ is transformed, if a point P of 7 is replaced by the points 
P’, which form a quadruple with ?; for the sake of brevity we 
shall speak of the transformation (P, P’). If we pay attention to the 
intersections of 7 with ?;” and with d,°, we arrive at the conclusion 
that @ has nonuple points in B, and triple points in Dy. It has 
therefore with a gy in 4, 81 points in common; further these 
curves cut moreover in the three triplets which correspond with the 
intersections of ? and 7. Consequently 9 is a curve of order thirty. 


104 


On an arbitrary straight line lie therefore fifteen pairs of cotangential 
poms. 

By the transformation (P, ?’), the curve 2", which contains the 
linear triplets, is transformed into a figure of order 1350. It consists 
of twice 2 itself, three times «, twelve times the curves B® and 
seven times the singular curves d*. For 2 x 45+3 «12+4+9x 
12 < 91098; the points PD produce therefore a figure of order 


252. From this it ensues that 4** has septup/e points in the 12 singular 
points D. 

The pairs P, P’, which are collinear with a point &, lie on a 
eurve «*, on which / is a triple point; the tangents in # go to 
the points of the triplet of the (P'), determined by /. The line HA, 
cuts p,’ in 9 points P, which form with 4; pairs of the (/*) ; hence 
e* has nonuple points in By. 

The locus of the pairs P", P", belonging to the pairs P, P’ of 


e'’, we shall indicate by «,. As # is collinear with 12 pairs of the 


involution (/*) lying on 2,°, B, is a dodecuple point of &,. 


On an arbitrary g* the cotangential points form three involutions 
of pairs and the supports of the pairs of each of those involutions 
envelop a curve of class three (curve of Cayiny). Consequently 1 
is collinear with 9 pairs P, P' of ~’, and this curve contains 9 pairs 
of s. As the two curves in 4; have moreover 9 >< 12 points in 
common, consequently 126 points in all, e is a curve of order 42. 

The curves ¢** and B,° have in the points 5,(4==1)8 x9 3 
points in common; moreover they meet in 9 points of #4, and in 
the 12 pairs P, P' mentioned above. The remaining 48 common 
points must lie in D,; so e* has quadruple points in the 12 singular 
points D. 

The curves «,‘? and 8° have in By (k==1)8 x 12 <3 inter 
sections; further they meet in the 9 pairs P", P", belonging to the 
9 points P' lying on #B,, and in the 12 points P", belonging to 
the 12 pairs P, P’ of 3,°, which are collinear with 4. So they must 
have 60 intersections in Dj); &"* has consequently quintuple points 
in the 12 singular points D. 

The curves ¢,"* and «” have in Be 9X 123, in D,12K5K2 
intersections, together 444; the remaining 60 lie in points of infleetion, 
of which the harmonic polar lines pass through /. In sueh a point 
of inflection /, «&,? will have a ¢rip/e point, for the corresponding 
3, 80 that 
T appears three times as point of ¢&,. Consequently 4 bears 20 
straight lines h: the harmonic polar lines of p* envelop a curve of 


polar line h contains a linear triplet, so three pairs of & 


class twenty. 


105 


Mathematics. — “A cubic involution of the second class.” By 
Prof. Jan pr Varins. 


(Communicated in the meeting of April 24, 1914). 


1. By the class of a eubic involution in the plane we shall 
understand the number of pairs of points on an arbitrary straight 
line’). In a paper presented in the meeting of February 28", 1914 °*) 
I considered the cubic involutions of the jirs¢ class, and proved that 
they may be reduced to sév principally differing sorts. 

The triangles A, which have the triplets of an involution of the 
first class as vertices, belong at the same time to a cubic involution 
of lines; the sides of each 4 form one of its groups. 

The cubic involntions of the second class possess the characteristic 
quality of determining an involution of pairs i.e. an involutive 
birational correspondence of points. For, let Y, ¥’, X" be a group 
of an involution (X*°) of the second class; on the line X’ NX" lies 
another pair Y’, Y""; the point VY’, completing this pair into a triplet, 
is apparently involutively associated to XY. In the following sections 
I shall consider a definite (Y") of the second class and inquire into 
the associated involutive correspondence (\)’). 


2. We start from a pencil of conies g? with the base-points 
A, B,, B,, B, and a pencil of cubies ¢° 
B,, CG. (h=1 to 6). The curves «* and y 


arbitrary point Y, intersect moreover in two points X’, X", which 


with the base-points B,, B,, 


*, which pass through an 


we associate to A. As the involutions /* and /*, which are determined 
on a Straight line by the pencils (4*) and (¥*), have two pairs X’, 
X" and ¥Y’, Y" in common, a cubic involution (X*) of the second 
class avises «here. 

The ten base-points are singular points, for they belong each to 
1 


0 
point of one of the pencils. 


groups; on the other hand is a singular point certainly a base- 


The pairs of points which with the singular point A determine 
triangles of involution A, lie apparently on the curve «* of the 
pencil (~*), passing through A. As they are produced by the pencil 
(¢?), they form a central involution, i.e. the straight lines.« = X’X" 
pass through a point Lot a (opposite point of the quadruple 
AB,B,B,). 


Analogously the pairs \’, 


i] 


, which are associated to C),, lie on 


1) This corresponds to the denomination introduced by Capora.i for involutive 
birational transformations. (Rend. Acc. Napoli, 1879, p. 212). 
*) “Cubic involutions in the plane”. These Proceedings vol. XVI, p. 974. 


106 


the conie y,2 passing through C,, which conic belongs to (y*); the 
straight lines v intersect in a point J/,, the centre of the /?. 

In order to find the loens of the pairs, corresponding to B,, we 
associate to each g* the gv, which touches it in B,. The pencils 
being projective on this account produce a curve of order five, B,°, 
which has a triple point in B,, nodes in B,, B, and passes through 
A and Cy. If the straight line «= X’Y" is associated to the straight 
+ and) qos niineeemes 
correspondence (J, 1) arises between the “curve of involution” enveloped 


line, which touches the corresponding curves » 


by a and the pencil of rays B,; from this it ensues that (7) must 
be a rational curve. As no other lines w can pass through 5, but 
ihe tangents at 3,° in the triple point B,, (z) is a rational curve of 
the third class, has consequently a bitangent; on it lie two pairs of 
(X*). To the tangents of (2), belong the lines Ab, and AB,. 

There are three singular straight lines b; = ABg; each of them 
bears a /* of pairs Y', XY". The corresponding points X lie on the 
ine nO bens 


8. The curve of coincidences (locus of the points X=  X') has 
triple points in #; and passes through A and C;. With the singular 
curve y*, it has 10 intersections in A and Sz; as it touches it in 
C’, and at the same time contains the coincidences of the involution 
(X', X") lying on y?,, it is a curve of order seven’), which will be 
indicated by 47. It passes through the 12 nodes of (y*) and the 3 
points (0; bin). 

As d@ has six points in common with g*, apart from By, and Ch, 
the involution /* of the A inscribed in g* possesses sev coincidences. 
In the same way it appears that the involutions 7? lying on «* and 
8° possess four coincidences each. 

The supports of the coincidences envelop a curve (d) of class 
eight; for through A pass in the first place the lines dg, each bearing 
two coincidences, and which consequently are bitangents of (d) and 
further the tangent in A at «@*, which will touch (d) in A. 

4. To the points Y of a straight line / correspond the pairs of 
points YY’ and XV" of a curve 2, which has in common with / the 
two pairs of the (.Y*) lying on /, besides the points of intersection 
of / and 6’; hence 2 is a curve of order eleven. By paying attention 
to the intersections of / with the singular curves a‘, B;°, and yj’, 
we see that 2'! passes three times through A, jive times through By 
and two times through C4. 


1) This corresponds to this well known proposition : the locus of the points where 
a curve o” of a pencil is touched by a curve ¢” of a second pencil is a curve 
of order 2(m--n)—3. 


107 


On 2, XN’ and X" form a pair of an involution; of the straight 
lines v= NX’ X" six pass through A. Three of them are indicated 
by the intersections Y of / and «'; here ’ lies every time in A. 
The remaining three are the lines 6;; for each of them contains a 
pair X’, Y" corresponding to the point Y = (/b,,,,). 

The curve (x), enveloped by w is rational, because we can associate 
w to NX; it has therefore ten bitangents. As such a bitangent bears 
two pairs \’, X" and Y’, Y" it follows that the imvolution (X,Y) 
contains ten pairs on /, and consequently is of the tenth class. 

5. Let a straight line / be revolved round a point HL; the pairs 
X', X" and Y', Y" lying on it describe then a curve «°, which 
passes twice through / and is touched there by the straight lines 
HE and HE". On EFA lie two points X' and Y", each forming with 
Ea pair of the (X"); so A is a node of ¢°. For the same reason 
é° has nodes in 4;; it also contains the points Ci. In consequence 
of the existence of 5 nodes, &° is of class 20, so that / lies on 16 of 
its tangents. Of these 8 contain each a coincidence of the (Y*); the 
remaining 8 are represented by four bitangents, being straight lines 
s, on which both pairs belonging to (X"*) have coincided. From this 
it ensues that the lines s envelop a curve (s), of the fourth class. 
Apparently the straight lines s, passing through A, are tangents to 
a’. In the same way the four tangents out of A, to pe° are the 
straight lines s, which may be drawn through By. ts 
and J’ have 16 points in 


6 


Apart from the singular points ¢ 
common; to them belong the 8 coincidences of which the supports 
d pass through #. The remaining 8 must be points Y’, coinciding 
with the corresponding point Y without ¢/’s passing through 4; i.e. 
they belong to the locus «, of the points Y, which complete the pairs 
lying on é* into groups of (.X°). 

As EF lies on three of the straight lines «= X'NX" belonging to 
br, By is a triple point of e,; analogously A and C; are simple 
points of that curve, so that the latter has 2+3<2<3+6= 26 


6 


intersections with ¢° in the singular points. Besides the 8 points of 


7 y 
' ny 


J’ indicated above they have moreover the points 4’, £” in common; 


so we conclude that «, must be a curve of the sivth order. To the 
intersections Y of ¢°, and / correspond lines w, which pass through 
HL; trom this it ensues again that v envelops a curve of the sixth 
class, when Y deseribes the straight line /. 


6. If # is laid in C,, &° is replaced by the tigure composed of 
1 | \ : 


> and a curve y,*, which has a node in C,, 


the singular conic y, 
and passes through the points A, 5;, C,. The two curves have apart 


108 


from A and Be two more points “’, 2" in common; the lines 
C, £', C, #" touch y,.in C, and are apparently the only possible 
lines s passing through C,; hence C, is a node on the curve (s),. 

The curve ¢." belonging to C, is represented by the figure com- 
posed of y,* and a curve *y,*, which has nodes in Ly. This may 
be found independently of what is mentioned above. The trans- 
formation replacing a point Y by the corresponding points X', X", 
transforms a straight line / into a curve y1', consequently the curve 
y,' into a figure of order 44. It consists of y,* itself (for this curve 
bears oo’ pairs X, X'), twice ,?, the curves a’, B;° 7,’ and twice the 
locus of Y"; the latter is therefore of order four. 

If # is brought into the centre J/, of the 7? lying on y,?, &° passes 
with node J/,. Of the latter 6 tangents 
pass through J/,, whereas this point lies on 2 tangents of y,?; from 


into y,? and a curve ,,* 
this it ensues anew that the lines d envelop a curve of the eighth 
,' four points in 
common, which must form two pairs of the /?, and so determine 
two lines s, J/, too is a node of the curve (s),. 

If # lies’ in A, &° consists apparently of a@’*, and the three lines 
b.; whereas ¢,." is the figure composed of an @ and the three lines 
bun. For FE in T &* is replaced by the figure formed by a® and a 


class. As y,? apart from A and 4, has with u 


curve t*, also passing through 7’ and having with a@* besides the 
four points A, By. two more pairs collinear with 7’; consequently 
T is also a node of (s),. 

For Bb, «° consists of B,° and the line BA; «,° of B,° and B,B. 

7. Passing on to the consideration of the involutive correspondence 
(X, 1”) we cause X to describe the straight line /, and we try to 
find the locus of the corresponding points Y. On each line X' X" 
lies a second pair J’, Y"; the curves ¢* and g*, which intersect 
in the points }', Y" we shall associate to each other. In order to 
determine the characteristic numbers of this correspondence, we 
consider the involutions /°, which are formed on a curve ¢ or g* 
by greups of (X*). 

The sides of the 4 described in a ¢ envelop a conic; among 
the 12 tangents, which this curve has in common with the curve 
of involution (wv), belonging to 4'' must be reckoned the two lines 
N\', X", for which X is one of the intersections of / and g*. The 
remaining JO contain each a pair Y', ""; consequently each g? is 
in the said correspondence associated to 10 curves gp’. 

The involution /* on a y* possesses a curve of involution of the 
third class; for 6, bears in the first place the line 6,, which contains 


109 


a pair of the 7*, then the lines joining B, to the two points, deter- 
mined by the y*, which touches y* in 5,. The intersections of / 
and g* procure three common tangents of (7), and (v),; there are 
consequently 15 straight lines, which bear a pair )”', Y"", so that 
the said correspondence associates 15 curves ¢° to y”. 

By means of this correspondence the points of a straight line + 
are arranged into a correspondence (30, 30). For to the gv? passing 
through a point R of 7 correspond the 30 intersections A’ of 7 with 
the 10 curves g* associated to g*; on the other hand the g* passing 
through =f’ procures 30 points A, by means of the corresponding 
15 q’. The intersections of the corresponding curves form therefore 
a figure of order 60; it consists, however, of two parts: the locus 
of the pairs ¥’, ¥", which lie on the tangents of the («),, and the 
locus of the points Y. 

The former may also be produced by. the pencil (v*) and’ the 
system of rays (v),. To each y?, in virtue of the consideration men- 
tioned above, a number of ten straight lines is associated, which are 


each coupled to one yg’ only ; henee a (10,12) arises now on 7, so 
that the pairs of points ’, Y" are lying on a figure of order 22. 

For the points )” we find therefore a figure of order 38; it is 
composed of the three lines 4, and a curve of order 35. For to 
the intersection Y of / and 6,24, corresponds a pair XY’, VY" on AB,; 


but this line bears co! 


pairs ’,)"" and the corresponding points 7 
of b,B, are all associated to V. Apart from these three lines the 
line / is transformed by means of the birational correspondence 
(X, Y) into a curve of order 35, 7**. It cuts / in 10 pairs_X, Y (§ 4) 
and in 15 coincidences Y= )’. There is consequently a curve of 
coincidences of order jifteen. The figure of order 22 found above 
1 


consists of the three lines 6; and a curve 4'', for to the conic (,, O,,) 


corresponds the tangent , of (),. 


8. We shall now determine the fundamental curves which are 
associated to the fundamental points A, By, Ch. The curves of invo- 
lution (7), belonging to ¢,° and 3,° (§ 2) have 9 tangents in common, 
there are consequently 9 lines, for whieh lies in , and Vin £,. 
Therefore the fundaniental curve of 2, has nonuple points in 2, and 
B,. No other point VY of the line B,6, ean correspond to a point 
X lying in £,; the said curve is therefore of order 18. It has a 
nonuple point in 4 too and passes three times through each of the 
points A and C),; for through 7 or J/;, passes one line, bearing a 
pa ie, eof py and aspair YY" 
then 5, = X corresponds to a point Y lying in A or C4. 


of «@ or xy)”; through whien 


110 


The fundamental curve of A is apparently identical with the 
curve &" (§ 5) belonging to the point 7; we shall indicate it by a’. 
As «* has two pairs in common with t* (§ 6) A is a node of a’. 
That «® passes through the points Ci, and has triple points in Bz, 
ensues from the consideration of the lines 71, and of the tangents 
out of 7’ to the (xv), belonging to By. 

It appears analogously that the fundamental curve of C, has 
triple points in 4; and a node in C,; it passes through A and the 
remaining points C, and is of order six. This curve is at the same 


6 


time the «° belonging to J/,. 

We can now prove once more that the birational correspondence 
is of order 35. To the intersection Y of two lines /, corresponds . 
the point }’, which the two curves 4, apart from the fundamental 
points, have in common. As appears from what was mentioned 
above 2 passes 18 times through 4; and 6 times through A and 
Cy; from 1+ 3 187+ 7 6? = 1225 = #5? it appears now that 
2 is a curve of order 35. 


Physics. — “On the manner in which the susceptibility of para- 
magnetic substances depends on the density.” By Dr. W. H. 
Knpsom Supplement N°. 36c¢ to the Communications from the 
Physical Laboratory at Leiden. Communicated by Prof. H. 
IKCAMERLINGH ONNES. 


(Communicated in the meeting of April 24, 1914). 


§ 1. Introduction. In Suppl. N°. 32a (Oct. °13) an expression was 
developed for the molecular rotatory energy in a system of freely 
rotating molecules as a funétion of the temperature. This expression 
was introduced into the theories of Laneryin and Wrauiss, on the sup- 
position that, when the equipartition laws are deviated from, the 
statistics of the molecules under the action of an exterior directing 
field, in this ease a magnetic field, is determined by the value 2, of 
the rotatory energy in the same way as for equipartition it is by 
‘kT. Wt then appeared that different experimental results can be re- 
presented very satisfactorily in that way '). 

1) The expressions developed in the above-mentioned paper appear to be also 
suitable to give a quantitative representation (as far as observations are available) 
of the decrease of the temperature of the Curin-point by the addition of a dia- 
magnetic metal to a ferromagnetic one, with which it forms mixed crystals, on 
the supposition that the diamagnetic metal exerts no other influence than that the 
vautual action of the ferromagnetic molecules is lessened in consequence of the 


sale 
In the communication mentioned above the system of molecules 


increase of their distance, as regards the molecular field in particular according 
to the supposition mentioned further on in this note. In fig. 1 the points -++- repre- 


~ 


Fig. 1. 
sent the temperature 7» of the Curte-point of alloys of nickel and copper as a 
funetion of the mass-composilion «x of nickel according to W. GuerTLer and G. 
Tammann, ZS anorg. Chem. 52 (1907), p. 25 [the quantity « introduced here is 
not to be confused with thal ef equation (4)|. The carve represents the results of 
the calculation. In this I started from equation (16) of Suppl. N°. 32a, applied to 


the nickel molecules 


Nnngu? 
= Uae oteeney Nes! Wem <M (sete sci fee ah (cz) 


3 
The density of the different alloys of nickel and copper was assumed to be equal, 
so that the density of the nickel in the alloy may be put equal to @ = 9,2 (the 


index 1 indicates that the quantity concerned corresponds to «= 1, that is in our 
case to nickel’. Further the coefficient of the molecular field, Nm, is assumed not 
to depend on the composition. This assumption involves, that the molecular field, 
the magnetisation per unit of mass being kept constant, ’s proportional to the first 
power of the density of the ferromagnetic component; this relationship differs 
from the result obtained by Wetss, G.R. 157 (1913), p. 1405, with alloys of the 
two ferromagnetic metals nickel and cobalt from the manner in which the con- 
stant of the molecular field, derived on the assumption of equipartition, depends 
on the composition. 
Further @, has been put (cf § 5 of this Bape proportional to 27/s : 
Ay = A, 1 av : > F, = c - (d) 


The equation which determimes the value of Te which cateeennaas to a given 


112 


was always‘) supposed to be contained in the same volume. and 
in the comparison with experimental data no account was taken of 
the influence which the relatively small changes of density connected 
with the temperature changes exert on the parameter (/,, which 
acenrs in the formulae of that communication, and which [ will 
call the characteristic zero-temperature. 

Since then the measurements by Prrrimr and Kaweriincu ONNEs *) 
coacerning the susceptibility of liquid mixtures of oxygen and nitro- 
gen have furnished very important data, which, when considered 
from the point of view taken in the paper quoted above, allow a 
conclusion as to the manner in which the characteristic zero-tempe- 
rature @, depends on the composition of those mixtures. If it is 
further assumed with Prrrmr and KamertmGcu Onnes, that to a’ 
first approximation the presence of the nitrogen molecules in these 
mixtures does not exert a direct influence on the statistical distri- 
bution of the orientations, nor on the magnetic noment of the oxygen 
molecules, so that it is only the changes in density of the oxygen, 
which determine the changes in the susceptibility, then those mea- 
surements furnish at the same time data for a discussion of the 
question how “, depends on the density. 

We will in the first place treat the question whether the results 
of the measurements by Perrier and Kamuriincn Onnxes mentioned 
above can be represented with the aid of the relations of Suppl. 


value of 2, may then be pul into the form: 


Ure Urel 


== ails ec, ec a . (c) 


«0 UyO1 


Ota 
For nickel (7.1 = 633, G0,1 = 2100, cf. Suppl. N°. 32a § 4) awd 1,30. From 
UyO1 


i 


‘“ the value of can be derived, and then with “/) from (b) the value of 7c 


ae) 0 


corresponding to «2 can be found. 

A continuation of the investigation of the magnetisation of alloys such as those 
mentioned above, particularly for compositions, for which the CuRt&-point lics 
below O° C., would be of great interest, on the one hand for putting the appli- 
cation of the quantum-theory to a test (according to this with such alloys the 
different cases indicated in Fig. 5 of Suppl. N’. 326 might be realised), on the 
other hand for increasing our knowledge of the molecular field [In the mean 
time | nave received an article by P. Watss, Ann. de physique (9) 1 (Febr. 1914) 
p. 134, in which is mentioned, that, with a view to the investigation of the 
molecular field, a series of measurements concerning alloys of nickel and copper 
has already been undertaken. (Added in correcting the proof of the Dutch edition)]. 

') With the exception of the note added in Leiden Comm. : note 2, p. 6. 


*) ALB. Perrier and H. KAMeRLINGH ONNES. Comm. No. 139d (Febr. 714). 


113 


N°. 32a’). It is shown in § 2 that the answer is in the affirmative, 
in § 3 the same appears to be the case for the measurements con- 
cerning the susceptibility of liquid oxygen over a wider range of 
temperatures. § 4 contains the conclusion which follows from §§ 2 
and 3. Finally in the following § § are treated the consequences 
concerning the dependence of 6, on the density, which follow from 
the results of those measurements *). 


§ 2. The susceptibility of the liquid mixtures of oxygen and nitrogen 
and the application of the quantum-theory to paramagnetisin. As a 
preliminary to the question whether the results of the measurements 
by Prrrmr and KameriincH Onnes can be represented with the aid 
of the relations of Suppl N°. 32a, in so far as these are applicable 
to paramagnetic substances, the specific susceptibility of the oxygen 
in the mixtures (Table [, Comm. N*. 139d) was compared with the 
specific susceptibility for pure oxygen in the gaseous state at the 
same temperature, which would follow from the measurements by 
Weiss and Piccarp if Curim-LAnGrvin’s law remained valid down to 
that temperature (cf. tabie I, Comm. N°. 139d). This value we will 
call the equipartition value Zey. 

On the assumption mentioned in § 1, that the presence of the 
nitrogen molecules does not cause a change in the magnetic moment 
of the oxygen molecules, the (paramagnetic) specific susceptibility of 
the oxygen in the mixture is determined by Oostgruuis’s relation : 

nu 
Owmnmintre— gag Py (1) 


In this relation n represents the number of oxygen molecules 
in 1 gram of oxygen, uw is the magnetic moment of an oxygen 
molecule, w, the mean rotatory energy (about two axes 4 to the 
magnetic one) of a molecule of oxygen in the mixture at the tem- 
perature and density considered. According to LanGuvin 


nu? 
Xeq. = 3k" 
Division gives 


1) For a detailed discussion of those measurements on the basis of the assump: 
tion of a negative molecular field, as well as a consideration of the other cir- 
cumstances which may have an influence, we refer to the paper by Perrier and 
KAMERLINGH ONNES quoted above. 

*) The principal results of this paper were already inserted in the translation 
of Comm. No. 139d; p. 915 note 2 

8 

Proceedings Royal Acad Amsterdam. Vol. XVII 


114 


eq. Ur 
ee es me et CD 
kT 


Xo, in mixture 


If for w, we assume the temperature function, developed in Suppl. 
N°. 32a, and determined by 


- (4) 


where 
2 
0 
Ct —— g ké, ’ . : . . . . . . (5) 
: : Skip r 
at each value of « the mutually corresponding values of Ep ae 
r 0 


can be calculated. The value of ae corresponding to the value of 
: / j 
0 
u/kT given by equation (3) can then be found by graphical inter- 
polation, after which @, immediately follows. 
From the data of Table [| Comm. N°. 139d by Perrier and 
KAMERLINGH ONNES the following values of 6, were in that way 


obtained : 
TAREE | 
Values of J, | 
Oi) vs Sehr aaie | 
| 2 
| y  \f=— 195.65|f = — 202.23) = — 208.84) Mean | A (= a 9.) 
pera) Gob! | | 
1 | 0.7458 165 161 159 162 21.6 
I | | 
» HW 04010 | 975 99.5 | 971 98.0 13.1 
| WI | 02304 | 53.9 55.1 [61.0] 54.5 7.3 
SIV: s|Dlas0ele we 250 EYE || SPAN 23.3 3.1 
Vo 0.0801 7.55 10.6--} 91 1.2 
| | | | 


From the fact, that the individual values of 6, vary irregularly 
about the mean values, the conclusion may be drawn that the obser- 


115 


vations can be represented with suflicient accuracy by the equations 
(1) and (4). This is confirmed by Table Il which gives. the values of 
xy calculated with the aid of the mean values of 4, given in table I. 
Table II also contains the deviations ( C' between observed and 
calculated values. 


IPAS ELE II 


Calculated specific susceptibilities of oxygen. 
Comparison with observed values. 


| +i | 4 | i l 
| t= — 202.23) O-C || t= — 208.84, O—C 


0 |t=—195.65) O-C 
SS | ! ——— —— ——— 
1 |o7458 |} 2962 |—17 3139, | 06)| 2345. | £20 
eet hozofor! aa62) (|= 0.2\||" “s6l20 J 161) 300m - | 205 
| : MM | 02304 | 3636 |+ 05) 3038 |—os|| 4292 | [—5.7)| 
|= 1 | 01380 | ~ 384.6 |— 10] 4188 | + 1.6 || 460.1 | —03 | 
|v /ooso | 3037 | +12/| | WP a yaiey alleen pe | 


Table II confirms the conclusion that the observations concerning 
the specific susceptibility of oxygen in the liquid mixtures of nitrogen 
and oxygen can be represented within the degree of accuracy of 
those observations by substituting the expression 4:7’ in Lanarvin’s 
theory by an expression for the molecular rotatory energy which is 
derived from the quantum-theory with the assumption of a zero- 
point energy *). 

These observations do not therefore furnish a decision between the 
assumption just mentioned and that, in which the expression £7" in 
LanGEvin’s theory is left unchanged, but the assumption of a negative 
molecular field is added, which was found by Perrine and Kamernincu 
Onnes (Comm. N°. 139d) to be in sufficient agreement with the 
observations. In the mean time it must be mentioned that on the 
assumption investigated in this paper the inclination of the y~1, 7- 
lines for the mixtures with small density of the oxygen approaches 
to the equipartition value for oxygen, which follows from the measure- 


1) Dr. OostERHuts tells me, that calculations made in the way indicated above, 
but in which for a the expressioa is taken which was assumed by him in Suppl. 
N° 31, lead to the same result Cf. note 2 p. 915, Comm. N°. 139d 

8* 


116 


ment by Wetss and Piccarb, whereas, as was found by Prrrier 
and KampriincH Onnes, on the assumption of a negative molecular 
field with unchanged molecular rotatory energy a correspondence of 
the inclinations can only be obtained by the aid of a new hypo- 
thesis (unless the difference in inclination should be ascribed to a 
systematic difference of experimental origin). 


§ 3. The susceptibility of liquid oxygen and the application of 
the quantum-theory to paramagnetism. The susceptibility of liquid 
oxygen being measured over a considerably larger temperature range 
(from 65.°25 K. to 90.°1 K.: Kamertinch Onxes and Perrier, Comm. 
N°. 116; from 70.°2 kK. to 90°.1 K.: KAMERLINGH ONNuS and OosTERHUIS, 
Comm. N°. 132e), than was possible for the mixtures treated in § 2, - 
it is important to investigate whether the data which are available 
about liquid oxygen can be represented also with the aid of the 
relations (1) and (4). In table II] the corresponding data have been 
put together. 

As Perrier and Kamertincuo Onnns observe, account has to be 
taken of the change in density of liquid oxygen. For the reduction 
of 7, to the same density use was made of the result whieh will 
be derived in § 5 from the observations concerning the above mix- 
tures considered in connection with those concerning oxygen, viz. 
that at these large densities 7, is proportional to @”s. 


Tt AGB AE slita 


| Specific susceptibility of liquid oxygen 
(KAMERLINGH ONNES and PERRIER). | 
i | Keale.’ 1 | 
PI NEYR LOSE.) “ON TEC ore—=nio3. 3| O—-C 
| | Boal ey \with @, = 232. (ao 
| 4 (Gee) 
64.25 | 284.9 | 232.5 | 1.267 229 282.6 + 2.3 
70.86 | 271.4 | 232.7 | 1.235 | 233 | 271.7 70m 
| 77.44 | 259.6 | 231.3 | 1.204 | 238 | 261.3 =e 
| | | | 
0h i Watt 22012 | 1.143 | 232 | 240.9 ALO 
i | i : | a 
mean 232, 


The agreement between observation and caleulation may be con- 
sidered sufficient. This conclusion is supported by the observations 


117 


of KAMERIINGH ONNES and OosTERHUIS: 


TABLE Ilo. 


Specific susceptibility of liquid oxygen 
(KAMERLINGH ONNES and OOSTERHUIS). 


oO 3 
ii H.108 | Ao, = 232 (—~) epee OL=G 
10.2 Pat | 232.65 272 8 Oe 
| | 
79.1 258.1 297.4 | 258.8 Oa 
fe “O04 Se al 220.2 Dae. IL weleaie 
| i a> ae 


§ 4. Conclusion. The data treated in §§ 2 and 3 lead to the 
following conclusion : 

The susceptibility of oxygen in liquid mixtures of oxygen and 
nitrogen as well as that of liquid oxygen can be represented within 
the degree of accuracy of the observations with the aid of the 
application of the quantum-theory to paramagnetism as expressed 
by equations (1) and (4). 

The agreement between observation and calculation (particularly 
if the susceptibility of liquid oxygen is also considered over the 
whole range of temperatures) is somewhat better with the application 
of the quantum-theory than with the introduction of a negative mole- 
cular field alone: indeed Perrier and KamernincH Onnes find it 
necessary for the mixtures of oxygen and nitrogen also to change 
the value of the Curtm-constant. Calculations made for liquid oxygen 
support this conclusion. Nevertheless it is quite possible that for liquid 
oxygen also if a changed Cvrin-constant is assumed just as good an 
agreement may be obtained by the introduction of a negative 


molecular field. 


§ 5. Dependence of the characteristic zero-temperature on the 
density. Table 1V shows more particularly the manner in which /, 
depends on the density 9 of the oxygen. 

From the last column the conclusion may be drawn that for the 


, 4, 2 log 9, rs 

higher densities ——- approaches to #/,. For those densities we 
7 0g Oo 

may therefore write as a limiting law: 


G00; smn pay etch) << evel ete te. (Ol) 


0 


118 
TABLE IV. 


| | A log @, 


oO 4 ——— 
: sl) eAYogio 
San nn EE : 
0.0801 Oneal 
| ss 
0.1381 | 23.3 
| \) eale66 
0.2304 || 54.5 | | 
| | 1.06 
0.4010 | 98.0 
| 0.82 
0.7458 | 162 
| | Osan 


12235 ea) N2S2 un 
| 


where a is a constant (for a definite substance, This dependence 
of O, on the density quite agrees with that, which in Suppl. N°. 30a 
was derived for the molecular translatory motions from the hypo- 
theses assumed there, cf equation (184) of that paper. 
This result can be interpreted as indicating, that the proportionality 
factor in the relation 
C= eh, 
(ef. Suppl. N°. 32a § 2), in whieh e¢ represents the velocity of the 
“rotational waves” considered in the paper mentioned, is independent 
not only of the temperature but also of the density, as aceording 
to Suppl. N°. 80a equation (7) is the case for the corresponding 
“translational waves”. 
In Fig. 2 the points indicated by small circles represent the values 
of 6, derived from the observations as a function of e. The curve 
6—<— — Se pivese@o29) Sram 
| | | “| chosen so as to obtain agree- 
{| |} 6hcment for the higher valiies jor 
| | | | | | vy. This agreement is in fact 
| z4 | very good for @ >1, as results 
| from the fact that the two 
| curves do not intersect here at 
| a definite value of v, but coin- 
cide over a certain range of 
| densities. 
| | For values of @ smaller than 
1 a deviation begins to show 
Fig. 2. itself; this deviation at first 
increases regularly in proceeding to lower values of 9. 


119 


It is natural to ascribe this agreement at higher, and this deviation 
at lower densities to the following’). At larger densities the rotations 
of the oxygen molecules are continually disturbed by collisions, or 
at least interactions with the other oxygen molecules, so that the 
periods of revolution of the oxygen molecules cannot play a part 
in the determination of the frequencies in the system which govern 
the distribution of energy. 

For those densities the frequencies are determined by the analysis 
according to Jnans of the molecular rotatory motions in the system 
into natural. vibrations; the relations given in Suppl. N°. 32a § 2 are 
then valid as approximations. 

At small densities, however, at which every molecule performs 
in the mean a certain number of revolutions before its rotation is 
disturbed by the collision (interaction) with another molecule, it is 
the numbers of revolutions of the individual molecules in the unit 
of time which govern the distribution of energy. These frecuencies 
are then determined at the limit by Etnstwin’s relation *). 

Uy = 4 LD (2x)? 
and are independent of the density. 

Between these two extremes a transition range lies. 

If (for 7’ = 85) the number of collisions, which an exygen molecule 
undergoes. in 1 sec. at e=1 (the molecular diameter 6 = 3.10—-8 
derived from the viscosity), is compared with the number of revolutions 
per sec. (distance of the oxygen atoms being assumed = 0.7.10—%, 
derived from the moment of inertia calculated according to Hom‘) 
from O—1, which value was assumed according to Fig. 2 for 
oxygen in the gaseous state), one finds that in the mean the oxygen 
molecule makes 0.4 revolution between two successive collisions. It 
is, however, not necessary to assume that the number of times that 
the rotatory 


y motion is disturbed in a second, coincides with the 
number of times that this is the case with the translatory motion. 
Some room is thus left for an average number of revolutions between 
two successive disturbances of the rotatory motion other than the 
number just mentioned. But if we assume that the order of magnitude 
will not be essentially different, the result of the calculation mentioned 
above is such as to be quite consistent with the theory developed 


above that at g@=1 a transitional region begins in which the 


1) Cf. the note quoted p. 112 note 1. 

*) Rapports conseil Solvay 1911, p. 433. 

8) E. Hotm. Ann. d. Phys. (4) 42 (1913, p. 1319. The ¢ used by Houm 
corresponds to / in this paper. 


120 


frequencies of the individual molecules begin to play a part for the 
energy distribution. 

This theory involves that for smaller densities «, is no longer 
determined by the relations of Suppl. N°. 32a, equations (4) and 
(5) of this paper. Notwithstanding that, in consequence of the relative 
insensibility of the way in which w, depends on 7’ for the special 
assumption about the distribution of the frequencies (cf. Suppl. N°. 31 
§ 7 by Oosrprnuts), a good agreement may still be obtained by 
those relations with the observations considered in this paper, but 
then the values of 7,, which give such an agreement, do not have 
the meaning laid down by the theory in Suppl. N°. 32a, 

Meanwhile the part for the smaller densities (@ < 0.15) of the, 
@, ,o-curve of Fig. 2 may be given a simple meaning by supposing 


15 
the curve for this region to represent — A, if 4 is determined 
2 


by the fact that the u,,2-curve on the side of the high temperatures 
approaches asymptotically to 
uy kh (T + A). 


As according to the relations of Suppl. N°. 32a § 2 (ef. Suppl. 
4 
2) 
N°. 32) § 5) 0,=—A, the curve has also this meaning for 


o> 1. For a nearer interpretation of the intermediate region the 
theory will have to be further developed. 

On the side of the small densities the curve in Fig. 2 has been 
extrapolated (indicated by dots) to a part that terminates parallel 
to the c-axis, in agreement with the theory given above, that at 
small densities the frequencies of rotation are no longer dependent 
on the density. 

In this region of densities the rotatory energy is determined as in 
the simplified scheme of Estrin and Strrn or of OosTErauis, in 
which to all the molecules the same velocity of rotation was ascribed, 
or better in the more elaborate theory of Hotm'), in which the 


1) &. Houm. Ann. d. Phys. (4) 42 (1913), p, 1311. This theory, in which in the 
system of rotating molecules all frequencies occur, and for the distr:bution of the 
molecules according to the frequencies, in a way analogous tc that which PLancKk 
in his recent theory followed for linear oscillators, the plane in which the condition 
of a molecule rotatimg about one axis is represented by the values of its azimuth 
and moment of momentum, is divided into regions of constant probability limited 
[aes ; 3 
by energy curves 4=” ir 8 consistent with the resu’ts of ByerRum and EK. 
y. BaHR concerning the discontinuous character of absorption spectra in the 
infra-red of gases of not too high densities, if it is assumed that the absorption 


121 


distribution of the velocities of rotation over the molecules is taken 
into account. 

Resuming we may conclude, that the observations by PERRimR and 
KAMERLINGH ONNES concerning the susceptibility of liquid mixtures 
of oxygen and nitrogen, although they do not furnish an experimentum 
erucis between the theory of the negative molecular field and the 
application of the quantum-theory on paramagnetism, nevertheless 
fit without any constraint ') into the whole scheme which can be 
built up on the basis of this application. 


§ 6. The results of the former § concerning the dependence of 
6, on the density lead to ihe following inference regarding the 
influence of the rotatory motion on the external pressure. For those 
densities at which w, is determined by the equations (4) and (5), 
and at which 4, — 07s, the energy u, and also the entropy s, for 
the rotatory motion are represented by the same functions (only 
with another value of @,) as the corresponding quantities for the 
translatory motion in-an ideal gas. 

In that case the rotatory motion gives a contribution to the external 
pressure similar to that of the translatory motion. The ratio of this 
contribution, for one degree of freedom, to that which in an ideal 
gas is due to the translatory motion, approaches to 1 at increasing 
temperature *). 

At small densities, however, vz. in the region in which 6, does 
not depend on o, the rotatory motion does not give a contribution 
to the external pressure. This agrees with what has always been 
of radiation energy supplied from outside only occurs when the representative point 
has arrived at one of the limiting curves mentioned above (for instance in conse- 
quence of the probability of emission on reaching a limiting curve, cf. PLANCK, 
Theorie der Wiirmestralung, 2te Aufl., § 151, being changed by the presence of 
the radiation from outside) The observations by E. v. Baur, Verh d. D. physik. 
Ges. 1913, p. 1150, concerning hydrochloric acid seem to be mere favonrable to 
this view than to a distribution, in which, in the plane mentioned above, only the 


1 hy ? z : 5 . 
energy curves | m+ >} > are covered with points, which is the assumption 


alluded to in the note quoted p. 112, note 1. 

1) The views advanced in this § about the coming into the foregrond of the 
frequencies of rotation of the individual molécules are im fact, as will appear again 
in § 6, a necessary complement for small densities to the theory of Suppl. N°. 32a. 

*) I find that A. Wont, ZS. physik. Chem. 87 (1914). p. 9, by quite different 
considerations was also led to the suggestion that at large densities the molecular 
rotatory motion may give a contribution to the external pressure. (Note added in 
the translation). 


122 
derived for an ideal gas, e.g. from Borrzmann’s entropy principle, 
cf. Suppl. N°. 24a § 4, or from the virial theorem. Conversely it 
necessarily follows from this, that in Fig. 2 the 4,, e-curve at the 
small densities must change its direction to one parallel to the g-axis, 
as is clearly indicated by the point e = 0.08, 

In conclusion we will return for a moment to the assumption 
rigidly adhered to in this paper, zzz. that the presence of the nitrogen 
molecules does not exert any influence on the distribution of the 
rotatory energy of the oxygen molecules. The following mechanism 
would be in accordance with this supposition: the oxygen molecules 
behave at a collision (at least with the nitrogen molecules) as rigid 
smooth spheres, they carry a (magnetic) doublet (or have according 
to Suppl. N°. 324 § 7 a magnetic moment in consequence of a 
rotation about an axis of small moment of inertia with zero-point 
energy in the temperature region considered); the nitrogen moleeules 
have a_ structure such that they do not exert a directive force on 
the oxygen molecules. The object of this suggestion is, however, no 
other than to show that the assumption mentioned above is not an 
impossible one. 


Chemistry. — “Vhe Allotropy of Cadmium. IY’. By Prof. Ernst 
Conun and. W. D. Hertpprman. 


The electromotive behaviour of Cadmium. 


L. The dilatometric measurements made with cadmium which had 
been deposited electrolytically, had shown ') that this material is a 
modification which is not stable af room temperature. This corre- 
sponds with the result found by Ernst Conrn and E. GoLpscamipt *) 
in their investigations on the electrolysis of solutions of tin salts. 
When such a solution is electrolysed below 18° C. there is not 
formed grey tin as might be expected, but the modification whieh 
is metastable at this temperature is deposited. 
~ In the following pages we give an abbreviated account on the 
investigations we have carried out in order to identify the product 
which is formed during the electrolysis of solutions of cadmium salts. 


2. Some years ago Huxnrr*) deseribed “a low voltage standard 
cell”, represented by the following scheme : 
1) These Proc. p. 54. 


2) Zeitschr. f. physik, Chemie 50, 225 (1905). 
8) Trans. Americ. Electrochem. Society 7, 358 (1905). 


123 


| Solution of cadmium sulphate | Cd-amaleam 
* | of arbitrary concentration 12.5°/, of Cd by weight 

The electromotive force of this combination is 0.0505 Volt at 
25°.0. The reproducibility is about 0.5 millivolt. The cadmium elec- 
trode of this cell has to be electrolytically deposited, as Th. W. 
RicHarps and Lrwis') have proved, that only this kind of electrodes 
give a definite potential. Ernst Conn and Sinnien*), who used these 
cells in their piezochemical investigations also found that they are 
reproduceable. 


3. Some points in the construction of such cells which play an 
important role in the experiments, to be described below, may be 
given here. (Fig. 1 A). 


Fig. |. 


The glass part is a thin walled tabe about 8—10 mm. in dia- 
meter, closed at one end and provided with a platinum wire; two 
ov three centimeters above the closed end is a platinum spiral, with 
its end fused through the side of the tube (the wires are thoroughly 
cleaned with aqua regia before filling the cell). 

In filling, the spiral is pressed to one side and some 0.5 cc. of 
12.5 percent cadmium amalgam is brought into the lower part and 
melted (carefully avoid bringing the amalgam in contact with the 

1) Zeitschr. f. physik. Chemie 28, 1 (1899). 

*) Zeitschr. f. physik, Chemie 67, 1 (1909). 


124 


platinum spiral). The spiral is then pressed down into a horizontal 
position. The tube is now filled up with a solution of cadmium 
sulphate of arbitrary concentration (the E. M. F. of the cell is in- 
dependent of the strength of the solution). 

In order to produce the cadmium electrode a current of 1 or 2 
milliamp. (1 or 2 milligrams Cd per hour) is passed from the amal- 
vam to the platinum spiral. At least 18 milligrams must be depo- 
sited. The cell may then be sealed off. 


4. We specially call attention to the following passage in HuLEtr’s 
paper: ‘‘The electromotive foree of these cells is high when the 
cadmium 1s freshly deposited, and the length of time required to. 
reach the normal value seems to depend on the thickness of the 
deposit. Air free cells and those saturated with Cd(OH), behave like 
ihe others and I have as yet no explanation of the high E. M. F. 
of newly constructed cells.” Our table I shows this decrease of 
potential of newly constructed cells. It amounts to about 1 millivolt. 


POA BLE i: 


Temperature 25°.0. 
E. M. F. in Volts. 


ee —— 
eng | | 

TO cds ee | | 

5 > 2 After 1) After 2) After 3| After 4| After 5| After 7| After 8 
sont ates ae 

i 5 5 day days days | days days days days 
= vo 

= | Eo 

z| £ 

a. | 0.05156 | 0.05105 | 0.05084 | 0.05078 | 0.05070 | 0.05065 | 0.05052 | 0.05052 


| | 
b. | 0.05143 0.05099 | 0.05082 | 0.05076 | 0.05068 | 0.05067 | 0.05054 0.05056 
| 0.05154 | 0.05103 | 0.05084 | 0.05076 | 0.05070 | 0.05067 0.05056 | 0.05058 


0.05151 | 0.05099 | 0.05082 | 0.05076 | 0.05070 | 0.05067 | 0.05056 | 0.05056 


| 0.05162 | 0.05113 | 0.05090 | 0.05084 | 0.05074 | 0.05070 | 0.05058 | 0.05058 


S 


Ss 
~ 


5. These determinations and those to be described below were carried 
out by the PogecEnporrr compensation method. The resistances used 
had been checked by the Physikalisch-Technische Reichsanstalt at 
Charlottenburg-Berlin. The same was the case with the thermometers 
used. Our two standardelements (Weston) were put into a thermostat 
which was kept at 25°.0. We used as a zero instrument a Drsprez- 
p ArsonvaL galvanometer. It was mounted on a vibration free sus- 


125 


pension (Junius). The readings were made by means of a telescope 
and seale; 0.02 millivolt could easily be measured. 


6. As it was:very important for us to get rid of this variation 
of KE. M. F. we tried to find its cause. We thought it might be found 
in the electromotive behaviour of the cadmium amalgams, which has 
been studied particularly by H. C. Bur’). 

Fig. 2 contains his results as far as they play a role in our in- 
vestigations. The curves represent the E. M.F. (ordinates) of cells 
which are constructed according to the following scheme: 


Millivolts 


At. °/) of cadmium. 


Fig. 2. 
Solution of cadmium sul- 
Cd-amalgam F 
ee a phate (765.4 er. Cd SO He, SO, — He 
x-at. Proc. 2 pel Gas +7: 
/, H,O per Litre) 


The abscissae represent atom per cents of cadmium. 


oy Zeitschr. f. physik. Chemie 41, 641 (1902). 


126 


From the drawing it can be seen that the E.M.F. of these cells 
at 25°.0 is independent of the concentration of the amalgam when 
its concentration lies between 9.0 and 24.4 at.percents (i.e. 5.9 and 
15.4 percent by weight). As soon as the concentration decreases below 
5.9°/, by weight (when we pass from the heterogeneous amalgams 
to the homogeneous, (c.f. Bi1’s paper Fig. 3) the E.M.F. varies with 
the amount of cadmium present in the amalgam, the potential against 
pure cadmium énereasing with decrease in the percentage of cadmium. 


7. In the light of these facts the high E.M.F. of freshly construeted 
cells becomes intelligible. 

During electrolysis the cadmium which is deposited on the spiral 
is withdrawn from the upper layer of the 12.5°/, (or stronger) amal- 
eam, which was originally a two phase system. It is thus possible 
for this layer to become a monophase system and if this is the case 
the E.M.F. will increase when electrolysis is continued. After the 
formation of the cell its E.M.F. will then be too high. In the long 
run cadmium will diffuse to the upper layer: this becomes again a 
twophase system and the E.M.F. will decrease and finally becomes 
constant. 


8. In order to check this supposition we carried out the following 
experiment: We put two platinum spirals into the A-shaped tube B 
(Fie. 1). into the right-side tube we put some 1°/, (by weight) ead- 
mium amalgam (99 parts by weight of mercury, 1 part of cadmium). 
This amalgam is a fluid monophase system at ordinary temperature. 
We filled the tubes with a dilute solution of cadmium sulphate (half 
saturated at 15° C.). After this the cell was formed in the way 
described above. (1 milliampere). 

After having deposited 20 or 25 milligrams of cadmium on the 
left-hand spiral, the capillary tube on the right was brought into 
connection with a waterpump in order to remove the amalgam. A 
number of small pieces of the 12.5°/, amalgatn were then substituted 
for this. 

These cells give at once an E.M.F. of 0.0503 Volt when they are 
put into a thermostat at 25°-0 C. It is evident that our assumption 


oc 


made above (§ 7) is correct. 


9 All the cells we investigated have been produced in the way 
described ; it is now possible to measure their E.M.F. at onee with- 
out waiting for 8 to 14 days before their becoming constant. 


10. Our dilatometric measurements with cadmium which had been 


127 


electrolytically deposited gave the result that this material only under- 
goes transformation at temperatures below 100°, if it has been in 
contact at 50° (400°) with a solution of cadmium sulphate. 

The probable and obvious conclusion is that by electrolysis we 
get exclusively s-cadmium, the modification which is stable at high 
temperatures. If this were the case, the y-cadmium would be trans- 
formed into p-cadmium at 100°, into @-cadmium at 50° in contact 
with the solution of the sulphate. 

If now the y-modification is really generated by electrolysis, 
(analogous to what happens with solutions of tin salts) the Hunerr 
cells which have been measured until now would contain this 
material as the negative electrode. 

If this modification happened to be transformed into the modifi- 
cation which is stable at ordinary temperatures and pressures (1 atm.), 
this would manifest itself by a decrease in the E.M.F. 

On the one hand we are working in this case under extraordi- 
narily favourable circumstances for stabilisation (change into the 
a-modification) as the, material formed electrolytically is in a very 
fine state of division and surrounded by an electrolyte, while the 
quantity which has to undergo transformation is so very small 
(20 or 30 milligrams), that the transformation, if if occurs, will be 
finished in a short space of time. 

On the other hand, and this is to be borne in mind in researches 
of this kind, the possibility exists that the transformation which has 
to take place spontaneously, may be suspended, if the metal depo- 
sited by electrolysis forms only one single modification, as the germs 
needed for transformation are then absent. 


1i. That the stabilisation generally does not occur is shown by 
our dilatometrie observations as well as by many other facts i.e. by 
the experiments of W. Jancer,') Ernst Conen,*) Bun’) and Hunnrr,*) 
who all found the same E.M.F. (50 millivolt at 25° C.) for cells 
which were constructed according to the scheme: 


Cd | Solution of | Cd-amalgam 
electrolytically | cadmium ; 12,5 per cent 
deposited | sulphate | by weight. 


How obstinately the transformation may be delayed might also 


1) Wied. Ann. 65, 106 (1898). 

*) Zeitschr. f. physik. Chemie 34, 612 (1900). 

3) Zeitschr. f. physik. Chemie 41, 641 (1902). 

4) Trans. Amer. Electrochem. Soc. 7%, 333 (1905). — 


128 


be inferred from Hunerr’s') words: “many of these cells are still 
in good order after five years.” 

This wonld be in perfect accordance with our own experiences : 
Crark-cells which contain ZnSO,.6H,O as solid depolariser preser- 
ved their E.M.F. for five years notwithstanding their having been 
standing at room temperature, i.e. 25 degrees below the transition 
point of ZnSO,.6H,O. As in the case of Hunter's cells they had 
been sealed up after formation. 


12. On account of these observations it might be expected that 
even under circumstances favourable to a transformation (stabilisation) 
of the negative electrode only a certain number of Hurerr cells 
would show the transformation. 

On December 11'? 1913 we prepared three H.C. (N°. 1, 2 and 5) 
in the way described above (§ 3) at room temperature (80 mgr. Cd on 
the spirals). We then substituted a 12.5 percent cadmiumamalgam 
for the | percent. The E.M.F. was now 0.0503 Volt. After standing 
for two months at room temperature the cells were measured again 
on February 26% 1914. The E.M.F. of 1, 2 and 5 had deereased to 
00475 Volt at 25°.0 ©. and this value remained unchanged. As 
might have been expected the E.M.F. had decreased by stabilisation 
of the cadmium. 


13. We prepared two new cells (nos. 6 and 7) in the same way 
as 1, 2, and 5. Immediately after the preparation their E.M.F. were 
0.04847 and 0.04795 Volt respectively. Some days later these values 
became constant: 0.04788 and 0.04778 Volt. Stabilisation had begun 
already during electrolysis. 


14. In order to determine whether «cadmium is formed during 
electrolysis if, this modification is present on the spirals before electro- 
lysis begins, we shunted the cells 6 and 7 in a current of 1 milli- 
ampere. In this way we deposited upon the a-cadmium which was 
present, a fresh quantity of 30 mer. 

After formation we put a fresh (12.5 percent) amalgam into the 
cell, while a fresh solution of cadmium sulphate was also introduced. 

Subsequent to this treatment the E.M.F. at 25°.0C. was again 
0.05026 Volt which proves that y-cadmium had been formed on the 
old layer of «-cadmium. 


15. On continuing our experiments we found that on one oceasion 


1. Trans. Amer. Electrochem. Soc. 15, 435 (1909). 


129 


cells of O.047 Volt E.M.F, on another, cells of 0.050 Volt E.MF, 
were obtained. 

As our dilatometric measurements had shown that stabilisation 
occurs with great velocity at 50°, we prepared cells (C and O) at 
47°.9. The dilute amalgam was then taken out and an 8.5 percent 
(by weight) amalgam was put in, while a fresh solution of cadmium 
sulphate was used. We substituted an 8.5 per cent amalgam fora 12.5 
percent as our intention was to measure these cells also at 0° C.; 
At this temperature the 12.5 percent amalgam is a monophase system 
and such a system must not be used. 

In this way we found at 25°.0 C. 


Cell C: 0.04745 Volt. 
Cell O: 0.05022 __,, 


The cadmium in cell © had thus been stabilised at 47°.9. 


16. In order to check the results found up to this point we also 
determined the E. M. F. of our stable and metastable cells at 0° C, 
If the differences in E. M. F. at 25°.0 between the different cells 
were really to be ascribed to the presence of «cadmium (cell C) and 
y-eadmium (cell O) the difference which was at 25°.0 C. 2.8 millivolt 
ought to increase at 0° C. as we are at that temperature at a greater 
distance from the metastable transition point ¢-cadmium = y-cadmium. 

The measurements at 0° C. gave the following results: 


cell C: 0.05225 Volt. 
cell O: 0.05626 __,, 


While the difference was 2.8 millivolt at 25°.0 C. it has increased 
as might be expected to 4.0 millivolt at O° C. 


17. Several phenomena which are described by Hunerr, but which 
are obscure until now may find an explanation in the light of our 
experiments. HuLerr says: “A number of cells were made with addition 
of Cd (OH), thinking this might make a more uniform cadmium 
deposit; also the air was completely removed from three before 
sealing, and in others the air was removed and the cell saturated 
with nitrogen and with hydrogen. All of these gave very variable 
results, but in each case only 10 milligrams of cadmium had been 
deposited on the spiral, and | have lately learned this is too little 
cadmium, since some cells prepared as above described, excepting that 
only 10 mg. of cadmium was deposited on each spiral, showed the 
same irregularities and tendency to constantly decreasing electromotive 
force. These cells were recently all discharged and then reversing 

9 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


130 


the current about 26 mg. of cadmium was deposited on each platinum 
spiral, and they seem to be all coming together nicely and to the 
value indicated by the old cells”. 


18. Our observations agree perfectly with those of Hunerr but 
we have to add the following restrictions: A number of our cells 
in whieh only LO mgrs. of cadmium were deposited indicated imme- 
diately after formation an E. M.F. of 0.0502 Volt at 25°.0 which 
decreased during 2 days. Then it became constant: 0.047 Voit. 
Transformation into @-cadmium had consequently occurred; the faet 
that only a small quantity of cadmium is present causes the KH. M. F. 
fo reach very soon its definite lowest value. The phenomenon obser- 
ved by HuLrrr is therefore the quick stabilisation of y-cadmium. 


19. Prof. Hunterr has been kind enough to communicate to us 
ihe following facts: “Twelve cells which had been sealed after 
formation remained unchanged from March 18" 1905 to May 7 1914, 
i.e. during 9 years. Their EK. M.F. has been during all this time 
0,0505 Volt. The quantity of cadminm on the spirals varies between 
3.7 and 13.7 mers. of cadmium”. 


20. The decrease of E.M.F. which had been observed with cells 
which contain only 10 mers. of cadmium is consequently not to be 
ascribed to the minute quantity of metal’) deposited on the spirals; 
this quantity is much less in the cells which have been constant 
during 9 years. The reason of the decrease in E. M. F. of those cells 
is the transformation of y-cadmium into «-cadmium. 


21. In order to check this conclusion we prepared a number of 
cells (at room temperature) whieh only contained 5 mers. of cadmium 
on the spirals. Some of these remained metastable (0.050 Volt) while 
others were transformed into the stable form (0.047 Volt) after some days. 


22. Although the discussion of a number of questions must be 
delayed until a subsequent paper, we will mention here the behaviour 
of cadmium which has not been formed by electrolysis. 

In our second paper we stated that a piece of cadmium chosen 
at random which had been produced from the molten metal contains 
three modifications: «, B and y-cadmium. If such is the case, it might 


1) OpprBEcK found [Wied. Ann. 31, 337 (1887)] that a layer of metal A of 
2>10-® mm. suffices to give to a metal on which it has been deposited the 
potential of A. As the surface of the spirals in the H. C. was 0,28 cm? the layer 
of cadmium deposited is much thicker. 


131 


be expected that the potential of such a material against cadmium 
which has been formed by electrolysis should be zero. In erder to 
test this conclusion we carried out the following experiment: We 
prepared a certain quantity of electrolytic cadmium (Prep. A) (Comp. 
our second paper § 8) and determined (at 40°) the potential diffe- 
rence between this material in a solution of cadmium sulphate which 
was half-saturated at 15° C. and: 
1. Cadmium, which we received from KAnLBaum (molten) in a 
finely divided state (Prep. B). 
2. Cadmium which we had used in our dilatometric measurements ; 
in this material the presence of y-cadmium was presumed. (Prep. C). 
Making use of the small apparatus shown 
in Fig. 3 we first determined the potential 
difference between two samples of the same 
material, subsequently that between samples 
of different preparations. In this way we found: 
E.M.K. of A against A = 0.000037 Volt. 
a Be) eee B= 01000018) Volt: 
~C ‘A C= 0.00000 — Volt. 


Be MEK A 3 3 = 0.090037 Volt. 
Ae) C0 0000377 Volt: 
From these measurements we see that y- 
cadmium is really present in our preparations, 
Fig. 3. as the dilatometer had shown. 
Utrecht, May 1914. van “T Horr- Laboratory. 


(July 3, 1914). 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 
of Saturday June 27, 1914. 
Vou. XVII. 


DEce — 


President: Prof. H. A. Lorentz. 
Secretary: Prof. P. Zeman. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 27 Juni 1914, DI. XXIII). 


COW EE anes Se 


JAN DE Vries: “A triple involution of the third class”, p. 134. 

W. Kapreyn: “On the functions of Heruirs.”’ (Third part), p. 139. 

M. J. van Uven: “The theory of Bravars (on errors in space) for polydimensional space, 
with applications to correlation.” (Continuation). (Communicated by Prof. J. C. Kavreyy), 
p- 150. 

M. J. van Uven: “Combination of observations with and without conditions and determination 
of the weights of the unknown quantities, derived from mechanical principles.” (Commu- 
nicated by Prof. JAN DE Vrigs), p. 157. 

F. A. H. Scurememaxers: “Equilibria in ternary systems.” XVI, p. 169. 

A. Smits and 8. Posrma: “The system ammonia-water”. (Communicated by Prof. J. D. van 
DER WAALS), p. 182. 

N. G. W. H. Brercer: “On Hermire’s and Apev’s polynomia.” (Communicated by Prof. 
W. Kapreyn), p. 192. 

Ernst Couen: “The metastability of the metals in consequence of allotropy and its signi- 
ficance for Chemistry, Physics and Technics’. II, p. 200. 

Pu. Konuystamm and K. W. Warsrra: “Measurements of isotherms of hydrogen at 2C° C, 
and 159.5 C.” (Communicated by Prof. J. D. van per Waats), p. 203. 

K. W. Watsrra: “The hydrogen isotherms of 20° C. and of 15.5 C. between 1 and 2200 atms.” 
(Communicated by Prof, J. D. van pER Waats), p. 217. 

D. J. Kortewec: “The different ways of floating of an homogeneous cube”, p, 224. 

A. Wicumann: “On some rocks of the island of Taliabu (Sula-Islands)”, p. 226. 

F. M. Jascer and A. Simex: “Studies in the Field of Silicate-Chemistry”. II. On the Lithi- 
umaluminiumsilicates whose composition corresponds to that of the Minerals Eucryptite 
and Spodumene, p. 239. Ibid ILI. On the Lithiumaluminiumsilicates, whose composition 
corresponds to that of the Minerals Eucryptite and Spodumene. (Continued), (Communi- 
cated by Prof. P. van RompurGn) p. 251. 

E. Laqueur: “On the survival of isolated mammalia: organs with automatic function”, (Com- 
municated by Prof.,H. J. HampBurGEr). p. 270. 

C. A, Crommetin: “Isothermals of monatomic substances and their binary mixture:. XVI. 
New determination of the vapour-pressures of solid argon down to —205%.” (Communi- 
cated by Prof. H. Kameriincu Onngs), p. 275. 

Il. KaMErRtINGH Onnes: “Further experiments with liquid helium. J. The imitation of 
an AmprRE molecular current or a permanent magnet by means of a supra-conductor”, 
(Cont.) p. 278. 

H. Kamertinen Onnes: “Further experiments with liquid helinm. K. Appearance of begin- 
ning paramagnetic saturation’, p. 283. 


10 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


13 


W. Karreyn: “On some integral equations”, p. 286. 

H. G. van pe Sanne Banunuyzen, N. Winpesorr and J. W. Diererinx: “Comparison of 
the measuring bar used in the base-measurement at Stroe with the Dutch Metre No, 27”, 
p. 300. ; ; 

Hi. G. van pe Sanpe Baxuvyzen: “Comparison of the Dutch platinum-iridium Metre No. 27 
with the international Metre M, as derived from the measurements by the Dutch Metre- 
Commission in 1879 and 1880, and a preliminary determination of the length of the 
measuring-bar of the French base-apparatus in international Metres”, p. 311. 

L. K. Wotrr: “On the formation of antibodies alter injection of sensitized antigens”. 1, 
(Communicated by Prof. OC. Eyxman), p. 318. 

F. M. Jarcer: “The Temperature-coefticients of the free Surface-energy of Liquids at Tem- 
peratures from —80° to 16500 C. 1. Methods and Apparatus. (Communicated by Prof. 
P. van Romeuren). (With two plates), p. 329. 

F. M. Jarcer and M. J. Suir: Ibid If. “Measurements of some Aliphatic Derivatives,” p. 365. 
Ibid IIL. ‘Measurements of some Aromatic Derivatives.’ (Communicated by Prof. P. van 
RomeBurcn), p. 386. 

¥. M. Jarcer and Jur. Kaun: Ibid IV. “Measurements of some Aliphatic and Aromatic 
\thers”. (Communicated by Prof. P. van Rompuren), p. 395. ? 

F. M. Jarcrer: Ibid V. “Measurements of homologous Aromatic Hydrocarbons and some of 
their Halogenderivatives”, p. 405. Ibid VI. “General Remarks”. (Communicated by Prof. 
P. van Rompuren), p. 416. 

H. Haca and F. M. Jarcer: “On the real Symmetry of Cordierite and Apophyllite’. (With 
two plates), p. 430. 

P. ZEEMAN: “FRESNEL 
p. 445. 

J.J. van Laan: “A new relation between the critical quantities, and on the unity of all 
substances in their thermic behaviour’. (Conclusion). (Communicated by Prof. H. A, 
Lorentz), p. 451. 


s coefficient for light of different colowrs”. (First part). (With one plate), 


Mathematics. — “A triple involution of the third class.” By 
Professor JAN DE VRiks. 
(Communicated in the meeting of May 30, 1914). 
1. I consider the projective nets of conics represented by 
Qaz? + Mag? + aMaz = 0 and Ab.* + 16,2 + 26 — 
The points of intersection of corresponding conics form a quadruple 
involution *). 
On the straight line YZ, which we may represent by 2, = ey, + 
+ 6z;, the two nets determine the pairs of points, indicated by 


YA (Q’ay?+ 296a,az+o7a.2) = 0 and A (9%,? +200b,b.+-0°b.*) = 0. 
3 2 


These equations produce the same pair of points, as soon as the 
relations 


Day? = +t LAby?, LAayaz =e Zhbybz,, Dda.* = x1 > hb,’. 
3 3 3 3 3 8 


are satisfied. 
By elimination of 4,2',4" we find from this system the relation 
| Ay’ —tby", AyQz—tbybz, az’—tb* |= 0. . = 4 (2) 
1) This involution is an intersection of the linear congruence of elliptic twisted 


quartics, which I haye considered in my communication in vol. XIV, p. 1127 of 
these Proceedings. 


135 


trom which it appears that YZ contains three pairs of the involution ; 
the latter is consequently of the third class. 


2. We shall now suppose that the two nets have a common base 
point 4; they produce then a triple involution of the third class. We 
choose the base point 4 for vertex QO, of a triangle of co-ordinates. 

Through QO, pass o 


‘ conies of the first net, which are touched 


there by the corresponding conics. For we have the conditions 


Ss — > ‘ Sy) = SS 
Sr — 407 and 2 Na — t= be, 
3 3 3 3 


so that the parameters 4, 4,4” are connected by the relation 


aes 
aie Oued | 
3 3 . 
| — — [=== OL ies Voeomas cle ectperttig(()) 
eid a =b,,4 
3 3 
Now we find from (1) 
| Ie Ie 
|) ea Ge 
iL ete. 


| 
| 

| 12 "2 

| BE ose 


If we substitute these formulae 2, 4', 4" in (3), an equation of the 
eighth order will arise. The locus of the pairs Y', X" of the triple 
involution (Y*) associated to O,== A is therefore a curve of the 
eighth order, which we shall indicate by «&; A is a singular point 
of order eight. 

By (3) two projective systems with index two are separated from 
the two nets, which systems produce the curve «*. Their intersec- 
tions with the arbitrary straight line 7, are the coincidences of the 
(4,4), which the two systems determine on 7. If 7 is laid through 
A, the free points of intersection are connected by a (2,2); one of 
the 4 coincidences of this correspondence lies in A, because two 
homologous conics touch each other and 7 in A. Hence it appears 
that the s¢ngular curve a has a quintuple point in A. This corre- 
sponds to the fact that (V*) must be of the third class; the three 
pairs on a straight line 7 laid through A are formed by A with the 
ihree points in which 7+ is moreover cut by @*. The line «c= XX" 
envelops a curve of the fifth class; for of the system (x) only the 
lines which touch e* in A pass through A. 


3. A is not the only singular point of (X*). The homologous 
conics intersecting in a point Y are determined by 


Ziha,? = 0 and Pi ie 
3 3 


If these equations are dependent, JY becomes a singular point. 
10* 


136 
Through Y pass then two projective pencils of conics, which deter- 
mine a quartic represented by 
Qy> ax? bx? Ohare cnt re. ((24) 
or also by 
[B52 Gat Mast ie=Oh\ (212) 5 ees 
The singular points are determined by the relations 
Qy? ay" ay’ 
by? by? By 


[aoe 


Now the curves a,? 6,'? =a," b,? and a,’ 6,’? = ay’ 6,’ have apart 
from the point QO, (which is node on both) 12 points in common. 
To them belong the three points, which a,? =O and 6,7 = 0 have © 
in common apart from O,; they do not lie, however, on the curve 
ay" by"? = ay'" b,. There are therefore, besides the singular point A, 
nine more singular points By; the pairs of points, which form with 
ZB; groups of the involution (X*) lie on a curve {;*, so that By is 
a singular point of order four. 

The singular curve (;* is produced by two projective pencils with 
common base points A and ;; it has therefore nodes in these two 
points. From (4) and (5) it appears that this curve also passes through 
the remaining singular points. The straight lines 2, which contain 
the pairs X’,X’’ lying on s;', envelop a conic. 

As §,* passes through A twice, there are in (X*) two groups in 
which the pair A,45; occurs; so 5, belongs twice to a*. This singular 
curve has therefore besides its quintuple point A, nine more nodes 
Ey, is consequently of genus two and of class 18. 

On each of the 8 tangents of a*, passing through A, two pairs 
of the (X*) coincide; from this it ensues that the straight lines s 
on which two pairs have coincided, envelop a curve of class eight, 
which we indicate by (s),. 


4. We can now determine the order « of the locus 4 of the 
pairs of points X’, Y’’, which form groups of the (X*) with the 
points Y of a straight line / As a* contains eight points of J, a 
passes eight times through A; analogously it has quadruple points 
in By. The w points of intersection of 2 with an other straight line 
/* are vertices of triangles of involution, of which a second vertex 
lies on J, so that the third vertex must be a common point of A 
and 4*. As these curves, besides in two vertices of the triangle 
determined by the point //* and the w points mentioned, can only 
intersect moreover in the singular points, we have tor the deter- 


13% 


mination of 2, the relation 2? = «+ 2+ 87+9>< 4"; hence 15. 

The transformation (XY, X’), which replaces each point by the two 
points, which (X*) associates to it, transforms therefore a straight 
line into a curve of order fifteen with an octuple point and nine 
quadruple points. 

As 7 contains three pairs X,X’, which supply six intersections 
with 4’, the curve of coincidences Jd is of order nine. Apparently 
d* has a quintuple point in A and nodes in By. 

With a’, J’ has 56+ 9X 4=—66 intersections in A and B;; 
the remaining szv are coincidences of the involution of pairs lying 
on a@*. Analogously we find that /* has fowr coincidences on £;'. 

The supports d of the coincidences envelop a curve of the éenth 
class (d),,, which has a quintuple point in A. 


5. The locus of the pairs X’, X’’, which are collinear with a 
point /, is a curve «*, passing twice through 7 where it is touched 
by the lines to the points “” and #”’, which form a triangle of 
invoJution with /. It is clear that e* will pass three times through 
A and twice through each point 4; it is consequently of class 30. 

To the 26 tangents of «°, passing through /, belong 10 lines d; 
the remaining ones are represented by 8 bitangents, which are 
straight lines s. 

If EF is brought in A, then «* passes into «*. For a point 2, &§ 
consists of ~,* and a curve ¢;‘, which passes through A and the 
points 4; and has a node in 4; The two curves have 14 inter- 
sections in the singular points; the remaining two are points /’ and 
i’, belonging to = B;,. The 6 tangents passing through 2, 
at es; are supports of coincidences; the curve (d),,, has 2, for 
node. 

The curve «* has with d*® 51 intersections in A and #;; of the 
remaining common points 10 lie in the coincidences mentioned above, 
of which the supports d pass through /. Consequently there lie on 


é* 11 coincidences Y= X’, of which the supports do not pass 


through /, whereas \’ and X’’ are collinear with /. These 11 
points belong to the curve e,, which contains the points YX, for 
which the line «= X’X’’ passes through /#. The curves ¢«* and g 
also have ihe points 4” and /’’ in common, forming a triangle of 
involution with ££. As Z£ is collinear with 5 pairs of the /? lying 
on @* and with 2 pairs of the /* lying on Ly, &, passes five times 
through A and twice through #;. Consequently ¢° and «, have in 
all 3X5+9X2-+13=—64 points in common; the locus of X 
is therefore a curve «,*. 


138 


As EF is collinear with 5 pairs’) X’, X’’ of a’, and with two 
pairs of §2°, €* has a quintuple point in A and nodes in bg. 

If / is brought in A, &,° 

For £, &.° consisis of the curve 8,* and a curve *3,‘, which 
passes three times through A and once through the 8 points Bz. 

The intersections Y of «° with the straight line / determine 8 
lines w= N’N’’ passing through /; we conelude from this that x 
envelops a curve of the eighth class (1), when X describes the straight 
line J. In confirmation of this result we observe that with the 8 
intersections Y of / and «* correspond the 8 straight lines passing 
through A(X’’) to the associated points X’. 

As (/), must be rational, consequently possesses 21 dbitangents,. 
/ contains 21 pairs Y,¥, for which the corresponding points X7,.X7’; 


coincides with a’. 


V’,¥” are collinear. 


6. An arbitrary straight line contains three pairs (Y’, X"), (V7, 1"), 
(Z’,Z") of N*’; the corresponding points X, ’, Z apparently form 
a group of a new triple involution*), which we shall indicate by 
(XYZ); it appears to be of class 21. 

Apparently (XYZ) has singular points in A and B;. Let x be 
the order of the curve «, which contains the pairs }, 7, belonging 
to NA; let further y be the order of the corresponding curve 
b, belonging to Bg. 

Let the straight line 7 be described by a point 7, the associated 
pair X}” will then describe a curve 2, the order of which we shall 
indicate by z. If attention is paid to the points of intersection of 7 
with @ and ~;, it will be seen that 2 must have an 2-fold point in 
A, a y-fold point in By. 

In order to determine the numbers a, y, 2, we may obtain three 
equations. 

We consider in the first place the intersections of the curves 4 
and gw, which are determined by the straight lines /and m. To them 
belong the two points which form a triplet with dm, further z points 
Z, for which X lies on 7 and Y on m; the remaining intersections 
lie in the singular points. So we have the relation 

2 2) ee ae? Esa 5 eee 
Let the curve «a® be described by 7, then the figure of order 82, 
1) The curves g® and <-§ have 3X5+9X2X2=5!1 intersections in the 
singular points; they have 3 more points in common on FA; the remaining 10 
intersections form 5 points A’,X” collinear with £. From this appears anew that 
the curve of involution z® is of class 5. 
*) This property is characteristic of the triple involutions of the ¢hird class. 


135 


which is described by the pair X, Y, will be the combination of 
twice a’, five times a® and twice Bx. 
Hence 
SSS Gas bye ste So og eS ea a 6 l(t) 
If Z deseribes the curve *3,*, the corresponding figure of order 4z 
consists of the curve @,*, of three times @*, and of the 8 curves 


Bw (k £1). Hence : 


AV EY) ote og a, Oe a Ose Gs) 
Out of (6), (7), (8) we find by elimination of « and y, 
2? — Viz + 882 =0; 


so z is equal to 63 or 14. The second value, however, must be 
rejected ; for we have proved above, that (XYZ) is of the class 21, 
so that 7 has 42 points in common with 4 at the least. So we find 
the values 

z= 63, « = 40, i iis 

For the involution (YYZ), A is a singular point of order 40, 
B, a singular point of order 16. 

As 7 ana 4 besides the 21 pairs already mentioned can only have 
coincidences in common, the curve of coincidences (XYZ) is of 
order 21, Jd*’. 

Apparently a‘? has in A a 20-fold point, @,'° in Bz an eight-fold 
‘point; in these points d** has the tangents in common with «* and 3;.°. 

If X is placed in A and Y in By, c= X' X" envelops a curve 
of the 5t class, y= Y'Y"" a conic; so there are 10 straight lines 
a=y. From this it ensues that the singular curve @*° has ten-fold 
points in B;. In a similar way we find that the curve (;"* has 
quadruple points in /,; it passes ten times through A, eight times 
through Dx. 


Mathematics. — “On the junctions of Hermite.” (Third part). 
By Prof. W. Kaprryn. 


- (Communicated in the meeting of May 30, 1914). 


12. After having written the preceding pages, we met with two 
important, newly published papers, on the same subject. The first by 
Mr. H. Garsrtn: “Sur un développement @une fonction a variable 
réelle en série de polyndmes” (Bull. de la Soe. math. de France 
T. XLI p. 24), the second by Prof. K. Runer ‘Ueber eine besondere 
Art von Integralgleichungen” (Math. Ann, Bd. 75 p. 180). 


140 
In this section we will give their principal results though not 


altogether after their methods, and make some additional remarks. 


13. Mr. Garprun considers the question of the expansion of a 
funetion between the limits @ and 6, in a series 


fe) = AM, (a) + A, (a) +. 


where 
6 
el Ls 
A, = — —= [e—“7 (a) My (a) da. 
2°n!l Vax. ; 
a 


He finds that this expansion is possible when /(«) satisfies the 
conditions of Diricatrr between the limits a and J. This agrees 
with our result in Art. 7, the only difference being that our limits 
were —oo and +o. This difference however is not essential, for 
considering a function which has the value zero for all values 
a>a>b Art. 7 gives immediately the expansion of Mr. Garsrun. 

His proof rests on two interesting relations which may be easily 
deduced from the formulae in the first part of this paper. 

The first relation 


S Ay (#) Hp (@) ay alts Ay 43 (x) HT, (a) — H,, (x) Ay+1 (a) (29) 
Fp 2p! 2r+lp/ e—a 


may be establishedin this way. 
According to (5) we have 
2xHy 2) Sas x 2nH,—1 (x 
v LT, (a) Jal +1 (%) + n 1 (x) (n> 0) 
20H, (a) = Ap (a) 2nIT, - 1 (a) 
Multiplying these equations by H/,(a) and //,(2) we find by sub- 
tracting 
2 (@ —a@) A, («) Hy (a) = Ani («) An (a) — An (#) An-1 (2) 
— 2n|H, (#) Hy—i (a) — Hp—1 (x) I, (@)). 
Hence, putting for m successively 0,1,2,..n, we get 
1 | 2(¢-a)H,(«)H (a) = H,(x)H,(a)-A, (2), (a) 


(2(e-a)H, (@)H, («)=H, (a), (@)-H, (x) 1, (@)-2 |, (a) 41, (a)-H (x) 2, (a) | 


2(r-a)H, (a), («) =H, (a) H (a) -H,(a)H,(«) - 4[H,(w)H, (a)-H, (w) 1, (@)] 


—— | 2a) Hy (0) H, (a) =H 4.1(0)H, (0) Hye) 4 Ce) 
—2n| H,(a)H, —\(a@)-H" (2) H, (a) |. 


\ 


141 


in question 


Multiplying these relations with the different factors written on 
the left, the addition of these products immediately gives the formula 


The second relation 


zx 

ales Ga Vals | ¢ A 

See ee OES ee co. (30) 

1 27 nl 
0 

may be obtained by introducing (9) into the first member 

Thus we get 

T,(@)H,—-1(2) 
1 27. nl 

eon" wo 


ioe} u2 eo 
ial —— nm f : 
—— = e 4 u®cos | vu — — J|du J e—’v —! sin 
wu | Qin 2 
0 
where 


NIT 
vv — =) dv 
. 2 
1 wo yryr nm nx 
—2 cos{ wu — — }sin{| xv — = 
o 42". n! ( 2 ) ( 2 ) 
__ cos au sin xv eur iy sin wu COs VY %, urk+ly2k+l 
Fx ; Q2k (Qh) F ] Q2R+N(2h+ 1)/ 
uv uv uv uv 
cos au sin av (e2 +- e ® i sin xu cosav (e2—e 2 
re v ( 2 ) v ( 2 ) 
Substituting this value, it is evident, according to the formulae of 
Art. 6, that all the terms of this sum vanish except only the term 
corresponding to —1. 
Hence 


= H,,(«) ay 
= 


@ = 
oe COS LU SIN LV 
— du dv 
jl Qn nl ae v 5 
and because 
eb u? 
Ss Ji 
J e COBL DIGI —= Vor ean Ne ree Vn ence as (22) 
a 
0 
ea vp 
&, H,(a a ae 1 (coma sie 
er € dv. 
ae Qn, Rees v 
0 
If now we iply 
O and w, we hav 


multiply the equation (a) by dev and integrate between 
e 


149 


&® wu? 


x 
7 4 Stn eu af 
fe du=V ax | e-* de, 

u 


0 0 


thus finally 
HF 


5S Hr(e) Hn— Ce) == et f ee? da. 


1 22 nl 


0 


14. ° Prof. Rune gives the solution of the integral equation 


TF =| K (2) p(w -- 2) de <.5,2 eee 


where /(w) and A(x) are given functions and g (x) is required, by 
means of Hermire’s functions. 
He assumes 
K (x) = e—* [a, H,(x) + a,H,(x) + a,H,(2) + ...] 
gp («) = e—** [b,H,(2) ++ b,H,(a) + b,H,(@) + J 


which gives 


a 
J) = Gn be fe Hf, (x) e"t+2? HH, (u + «) dz 
or, after some reductions 
: 4 u 
Wm oo “(Ve 
(a) — = (— 1)"anbn : — =e 
i ) VAR th ( ) ; (V2 yntn 


If now, the given function f(w) is expanded in this form 


| u u 

"(u) = = ats cs (v2) ar : (v2) sie 
u) = —e Cy C, — Cy a 

i V2 V2 (V2) 


we have from (31) 


c) =a bn 3 16; = 0,000), 4) Cy =, 0s 10 Ge Oraienere 
and it is evident that from these relations the coefficients 4 may be 


determined. If /(w) and g(x) were the given functions, the same 
relations would be sufficient to determine the function A (7). 


15. The preceding reduction rests on the formula 


ie 1 
ET +) = —— [A,(2) + C."A-a(a)7,(y) + Cy" Ap—0(w) H,(y)4+. . 
wer 
+ C,,(y)) (32) 


143 


where C’ are the binomial coefficients. This relation may be obtained 
in the following way. 
According to Art. 8 Il we have 


. h? h® 
eens Th H, @) =le Dye (2) a 37 H, (<) ety ein ts) (p) 
and, expanding by Taytor’s theorem 
F(« +h, y + &) 


TA (a) ea ad 


l d 
e— (tk? —(y-+k)? et? +9? —er"-+7" | ev aey | e—y* al =) +e? ao ) | 
ai Y 


i ie Pads o 5 d is d ae et a e 
eye (eat ae [eee ey et : 
rary da? ‘ uF da \ dy ‘ By da? rs | - 


which may be written 


k? 
e— 2h 2h 1 AH (0) + Hy) +5 [A (0) 42110) (+H (0) 


where 


Putting now ¢ Seen (p) and k= no in.(g) we get 
V2 V2 
e-(a+yhve—l? — 1 —h H, (=) as = IT, (=) ect 
. h 
easy i218 — | Va [| H, (x) + A, (y)] + 
jE EG) Roe Gy 4 Fy ee 
(V2)72/ : 


hn 
Comparing the coefficients of — im the second members we obtain 
nh. 


the required relation (31). 
Proceeding to the reduction of the integral 


a 


M ee] EH, (w) e~2? IT, (u +a) da 


we put, according to (2) 


qn 
Lith (wv) —— (— 1)m ev oe (e-2") 


dam 
then 
xD 
>in 
, M= ip) ron OM) whe? Hh, (u +2) de. 
dat 


Now, integrating by parts we have generally 


i44 


in jin U 
fe a da=(— 1m firs dw + 
< ¢ Lym Lym 


+ | oS V dU dm—2V qm—1 U | 


Seo iy 


da dx dxm—* dam—1 


thus, assuming 
OG 6 =n) 


and introducing the limits —o and o 


= dm 
M =/e"= [e—utt? A, (uta)] da 
ain 


= (1)"fe-2 dutn —u+r)?) d 
— ) é damtn (e . ) v 
— (<1 fe —x2—(u-+xr)? et (u+-2) dz 
or, adopting 
—v 
uv V2 t= —— 
V2 
See - 
N= ames ap ad Antn (ee) dg. 
V2 V2 


Applying now the relation (32), it is evident that the integral 
reduces to the first term, thus 


(_D* pat An+n (v) 
V2 (VY Q)mn 


Uu 
Ue Tn, a7 
(-1)" ~2 (ys) 
= -—— e = : 
VY 2 (Vv g)mtn 
16. We will now compare the preceding solution of the integral- 
equation (81) with the formal solution given by Prof. K. ScHwarzscHILp 
Astr. Nachr. Bd. 185 N°. 4422). 
Putting 


MS 


or finally 


M 


Cer ey 18 Cae 
the equation 


fe (t.s) F'(s) ds = B(t) 
0 
takes the form 


145 


fA (e— (u+®)) F (e—*) e-* dx = B (e—*) 

or, assuming 

e—* F (e+) = K (a) 

A (e— (4) = o (uta) 

Ble) =f) 
{xe gp (u -+ «) dx = f(u). 
Now Scawarzscaitp multiplies this equation by e-’“ du and inte- 

grates between the limits —o and + o, thus 


[reo e—4u du =f ¢ (x) ae fy (uta) e—%u du 


= | K (ec) e* de fo (v) e—2” dv 


and puts 


2 i ,2 . 
Tw = fro eudu thus F (4) = 5— fren e— Pu du 
aT 


—o 


5 ier 
K (x) =z (a) e da x (2) = x I* (zie dx 
ast 


—D 


~ Pye ‘ 
@p (v) = Paedy , Bo()= ml @p (v) e—?” dv 
therefore 
F(A) = 2aL (—-A) ® (A) 
or 
Ky) : 


2x b(—1) 


LQ)= 


Multiplying again by e’*da and integrating between —o and 
+ o this relation, he obtains 
ei a) 
K («) = — ——_—— et dj. 
22.) b(—2) 


—o 


If now we compare this result with the preceding, we have 


146 


ee 
F(a)= xf eu du 


or 
u 
ar. 2 Ripe |e 5 a Wee 
F(a) 1 Ve ( — F NS (va) : 
b=— - CA Cy —— CF ae 5 du. 
on V2. ‘V2 (ar 


The general term in the series of the second member being 


u2 


Se } . Pay) ‘eo 
Jens = fe 2 IT, Ga e—44 du = V 2 fe 0? FT, (v) e742 dy 
V2 


—o —on 


it is obvious that for 2 = 24 the imaginary part and forn—=2k+1 
the real part of this integral vanishes. Thus for m= 2h 


i v2 | e—* Ao}. (v) cos (A v V2) dv, 


where according to Art. 8 IL 


2 
= Tops 2p 
os (AvV2)—e ~ S(--1)P ——— Ae, (v 
cos (Av ) é =i ) 2302p)! 2) (v) 
thus 
2k+1 2 


a ea 
Pop — (=a) 2 Vaaric mmaate 
In the same way, we get 


22 
Poppy = — i(— 1k 241 Ve 7 ARH 
and therefore 
32 
Y eT s% eee 
iC) = DS Po}. SS Ps 

\ ) 2V 27 Ok 2k u 2k+1 2k-+1 

2 2 
Biers s | 
= 58 [2 (— Mk ow Ei S (1h conga PE]. 


In the same manner we find 


® (2) = * [3S (1) bop 22!# — 2 S (—1)* borg BAH] 


Va 
and finally 


147 


2 


LC a Shoot iS (—1) hoop 12H 


ar : ex dx. 
rf S(—1)bad* piste ee 


If now the conditions 
SUNS C100 a0) c, =a,b, —a,b, + a,),, 
are satisfied, A(z) must be reducible to 
e— [a HH, (x) + a, H, (v) + a, A, (x) +...) 
It is easy to show, that this is the case; for if the conditions are 
satisfied we have 
D(—1)Fenp2 + iS (—1 hong 22k 41 


S(— yo! iS (— 1) EH a,?-+-a,2* ... —i(a,A—a,A*-+ ...) 


——n Ob 


0 


thus 
NY ey 
iKe(2)\— BV= Oe [> —1) ao, 2-1 (-1)F aon) A2AF1] (cos Ax + isinaa)da 
“Va 
2 2 
1 aoe. 
= ——_ | e * [cos Av XS (—1)' ap 2k + sind x S (—1)F agp 4 2k+1] da. 
Va 


or, introducing (9) 


=} = 
Hoy, (x) e-? = Gade € 4 yok cos Aw da 
Vae 


2 


ae apes 
Hox.43 (x) e—? = -—— e A2K+1 sin Ax da 
Vw 


K(#)=e = [a, ‘Hi, («),+ «, A, (#).+.2, Hf, (z) +... 
17. From the relation (32) another important result may be 


deduced. For multiplying by e—” dy and integrating between — o 
and o, this relation gives 


yH (224) 4 Va 
fe Jab (Se) a = (van 


ae+-y= aV 2 
eS 
(V2 )rh 


or, putting 
fave H,(a)da = H,(z). 


—o@ 


Therefore, assuming 


148 


1 = 
@;(a) = a 2 H,(w) 
22Y/nl x 
we obtain 
Q)rFl ( — —(Y—= ay?2 +23 
Cs (G)) = Vv = | e a 3 ein 
Va 


thus, in the same way as in Art. 9 
3 


= 1 gee 24 
By — — (a2—-—ary2+a3 
A= (V2), K(z,c) = Va Boe ( 3 i 


m 
Here the value of the function A’ (@.«) is finite for wand @ + o. 
In the same manner as in Art. 9, therefore 
es L)Ppn)a 
K(«,e) == nl“) Pn)@) 
0 an 
or 
e—(a2—2xa) 2+ Ce > H,(«) Hy(@) 
1 3n+1 
22 ni 


which may be verified by (9). 


18. Now, according to the theory of the integral equations the 
determinant D(a) of the kernel A(v,¢) must vanish for the values 
4=V2y41MmM=0,1,2..)). 

To examine this, we write D(a) in the form which is given by 
PLEMELJ ') 


Oe Pappa 3 
Se = (sea a GaP SE on: 
D(a) 1 2 as 
where 
a, = | K(a,2)dz2, af K (eae, a,—|\K,(@ x)da,..-: 
K,(a,@) = [Kew Ky—1(y,@) dy (n =1,2.3...) 
and 


K,(v.a) = K (a.a) 
From K (vy), which may be written 
K (ay) — Agha 2kay—ly* 


1) Monatshefte f. Math. und Phys. 1904 p 121. 


149 


the functions A,,(7y) which have the same form 


Ki, (xy) = Ane —hnax* + 2k, xy—lny’ , 


may be easily deduced, for 
ace 


K,(w.a) = AAy—1 fe (C+ hn) y? + 2(he + ky a@)y— (he? +1, 10° ) dy 


-@ 
and 
2) 7 oa) 
5 G2 fh gq \? 
: == =i j= = 
fe Sy 2gy—h dy ——/ On | é ( ) dy 
=o —o 
g—fh — 
ara 
=: ———— 
Vif 
Hence 
—h,v2+-2h,va—l,a@? 
A, é — 
ke? kkn—1 Re 
A —— == a? +2 : ca—| l4— ae a 
ee! = ( I+-hyn—1 Lt hy—1 i l+hy—1 


= V; e 
Vit hn ‘ 
which gives 
APA = ke k kn— 1 
u— —_— Vas hy=h— a a — ieee l,=l,-1— me : - 
Vhthy-1 la-hn—1 I+hy—-1 bt hy 


Now, we know 


4 : h i k=/y 2,1 8 
Jal SS oF OOS => ay — — 
Va Biv, 2 
thus 
i. 5 2 5 
A, == , kh ES — Se LS = 
V32 6 3 6 
1 9 2V2, 
A, =——= », 4, S — , 4 = - z neers 
Via 14 7 14 
1 17 4 17 


: “ Wiba 3 
and 
nH 
ee LA Bet A Eas ae Re ee 
Cn oon et Sk, 
This gives 
11 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


n+1 
2S 
~ as r? 
oy n+l i 
: Pp Penal ay ls 
QnA = fa (ez) dz = Veronad e af Cc =Ep 
9 2a 


Constructing now, according to Wee an integral funetion 
7(a), with the assigned zeros 
a= V2, 2=(V2)", 2 = (V2)... 


we obtain 


F@) = eG) (1 —— ,) 
F(9) n=0 (V2)n+1 
or, assuming 7(0)=1, G@a=0, a= r 
f (a) = IT (1—AorH), 
Thus ic 
Tita aes PO AR sk he 


70) Aa TS Ss 
and expanding the fractions of the second member 


Sep Se 2 =) OF 
7@ eae ry +4 ee ete An eas 
Comparing this with 
D(A) 
Giese At+a,vo+. 
we see that /(4)= D(A), tor (0) = DO) =1 and 
a Srp — i's = : : 
p= aa ppt np 
22 
Mathematics. — “The theory of Bravais (on errors in space) 


for polydimensional space, with applications to correlation.” 
(Continuation). By Prof. M. J. van Uven. (Communicated by 
Prof. J. C. Kaprryn.) 1) 


(Communicated in the meeting of April 24, 1914). 


In the theory of correiation the mean values of the products aja% 
are to be considered; denoting these by 77, we have 


1) The list of authors who have treated upon the same subject, may be supple- 
mented with: Cu. Mi. Scuots. Theorie des erreurs dans le plan et l’espace. Annales 
de |’Ecole Polytechnique de Delft, t IL (1886) p, 128. 


+n +o 
TT ae E : : —(b,.%"+ @it..+b ) : 
Vik = = =a UU € da, ..da 
n RP.) 
j= OX =—H 


To integrate in the first place over all the variables x except 
xv; and 2, comes to the same thing as to drop the g—2 linear 


relations x= Da; v;(/==7,4). Thus we start, as it were, only from 
1 
the two equations 


Bj = aziz + ajgve +... + ayers, 
Le = agiyvi + apgove +... + ager. 
and find therefore 


oo 2 ee 
pup +2 bi Ke jep + bpp’ eh?) | 
Yjik = LIL dajday , 
— oO U 
where 
E' == ES “ byy'; bik 
=p" Dik's Dick 


D’ yepresenting a determinant of the matrix 


Qj1y Aj2y +++ Aj 


| 
IE | | 
| cet 5 Qp2s +++ Akz | 
Besides 
i Ae Gia sss « Ofens 
Dy = aj, Aj2y 2 0 6 Ajay 
hence 
Day? 
pees TIS es 
bj; Sse = ES ap; ; 
oe = — EH Dajiapi; 
in. = E'S a5;7. 


By performing the integration we obtain for 1;% 


t =a 
ater bite = Aj Uk 
lik == ) 7! 9 


Sy? . 5 
z =v; Ma, — (bj j'aj? 4 2b ja jap ben’ 247) rire = Aji 
a vj dz ;* = — —. 
\n _ 
—@ —@ 


Now the correlation-coefficient 7;; of v; and a, is defined by the 
expression 
A hn 


152 


 — 


V nj ;%Kk 
This correlation-coefficient can therefore also be written in the 
following form 


> ajl al 
i —— — 
> aj". > axl” 
or 
By 
Vik 


V Bj; Bre 
Introducing the coefficients «;;, we find 


> €/? aj] Akl 


rik = —————————————— et) 
VS ef ae ae 

We now will imagine the variable w to be connected with some 
cause Q;. To express our meaning more clearly: we suppose the 
quantity 2 to be built up of some variables w, viz. as the sum 
of these variables, in such a way, that in this sum the term wy 1s 
lacking if ; is not subject to the influence of the cause Q. 

So in the relation 


Vj = aj, U1 + ajzue +... + aju +... + Qjz Us 
we have 
aji=1, when Q does act upon aj, 
aji= 0, when Qi does not act upon 2j. 


s 


Thus in 2 e? aj? only those terms &,*s &*)++-&,? occur which 


(— 
correspond to the variables u,,, u,,,...Ur,, due to the causes 
Oe GOR Weise Qn, actually influencing «;; on the other hand those 


terms are lacking, which owe their existence to the causes not con- 
tributing to 2;. 


In the sum 2 €/?aj;@% Only those terms &’ occur, for which both 
il 


aji=1 and az=1, that is to say: the terms, which derive from 


the causes (Q), acting both upon a; and zx. 


e 


The expression 1j;, = > &aj,a,, therefore may be called the 
i-1 


square of the mean value of those elements of «j and xk, which are 
due to the common causes. 


z,;, We may define the correlation-coefficient of the quantities 7; and 


av, in the following manner, proposed by Prof. J. C. Kaprnyn *). 

The correlation-coefficient rj. of x; and xp is that part of the 
square of the mean error common to «vj and aj, which is due to the 
common causes. 

Supposing every quantity w; to have the same mean error, or 

€; = €9 == ...=>=6& , 
we find for rz 
= aj) Ay) 


Hg Ni SS eT 
V Sa;)’. = ap? 
Now + a;,* apparently equals the number A; of the causes acting 


upon 2j, ay? the number NV; of the causes influencing x, and 


2 aj, ax, the number N,;;, of the causes contributing both tov; and x,. 
Jt Ek J 5 ‘ k 
Thus, in the case of equal mean errors, we have 


in other words: for ¢,=6#,—=...=e«, the correlation-coefficient 
equals the quotient of the number of common causes, divided by 
the geometrical mean of the numbers of the causes, which act upon 
xv; and 2, resp. 

If both xz; and zz are subjected to an equal number (V; = V;,—.V) 
of causes, Vj, of which act both upon 2; and a, then 
Nyx 
No 
in other words: the correlation-coefficient is that part of the causes 
of x; (resp. 2%) which also contributes to zz (resp. 2;). 


i 


The expressions for the correlation-coefficients admit of a very simple 
geometrical illustration. 

Calling spherical simplex S, a (g-dimensional) 9-gon lyeg on a 
g-dimensional hypersphere (extension of the spherical triangle in 
3-dimensional space) we may state that a spherical simplex |S. has 


9 (e—1) as 
—— edges pj, = Pj Pr. 


Gsavertices) 2 er. =... 3P, and 


Pp 


Opposite to the vertex P; we find, in the (@—1)-dimensional linear 
space a;, the (curved) (¢—2)-dimensional face of S,, which contains 
the remaining e—1 vertices P; (j=|=2). 

Further we denote by 2a), the angle between the linear spaces 
x; and a; [consequently also between the (@—2)-dimensional faces 


1) J. CG. Kapreyn. Definition of the correlation-coefficient; Monthly Notices of 


R. A. §., vol. 72 (1912), p. 518. 


154 


(Pi; Pa. se Pia Pha. PA and te Res en e ee 


Building the positive-definite determinant 


| 1 1 .€08)19) oh RCOSYPiS wy a= mismieenCOS OH om 
| 
| | 
cos P12; ] Te COSV0D3) uated i COSiDDD. 
r= 
cos Pig, COS P23 1 spn) eet SBCOS IS 
COS Pip , COSP2ap , COSPgo 3 - = - 1 | 


and representing by Cj, the minor of cos pyr, we have by the theory 
of the spherical simplexes 
: 
Ujk 
V Cy; Con 


cos Hj, = — 


Substituting 
big =H" bj = Gy Me C08 zk 

the quadratic form H in the expression for the probability W trans- 
forms to 

H = Bb 5; 0; + 2 Vd jK w; wp = ZV (qy aj)” + 2 > cos pju (95 %7) (Gk ee)- 

This form is positive-definitive, when 

r>0, 

or, in other words: when the arcs pj, are the edges of a o-dimensional 
spherical simplex. 


Furthermore 
P o ~ 
i —— GL 
1 
and 
i ° 
I V- 
1 Y 
Bip = ——_~ XK Cite 
qj Qk 
whence 
Byy. Cir 
i — Z g - == — cos IT;x,. 


VBij Bex  V Cjy Crt 
So, putting H in the form 
H = XJ (qj 2;)? + 2 = cos pjx (qj 7) (ge 2k); 
the ares pj; must be the edges of a 9-dimensional simplex and 
moreover: the correlation-coefficients are, but for the sign, equal to 
the cosines of the “opposite angles” IT;,. 
In the case of “errors in a plane” only a circle-biangle P,P, is 
to be considered. Then the are P,P, =p,, equals the angle J, 


11515) 


included by the opposite spaces (straight lines, radii of the cirele) 
a, = OP, and x,=OP,, O being the centre of the circle. 

So, in the case of two variables x, and x, with the quadratic form 

JE Oe tie PAO Cy Ol a= Opt re 
we have to put 
bi, =" 3 b,, = 49; ’ bb. =H G2 COS Py 5s 
whence 
E = q,’ 9," sin* p,,- 


The correlation-coefficient 7, now takes the value 


13 


b 


12 


i —— 1 COS ——|——1C08, Da — —. 


DVGe 


Considering the errors in 3-dimensional space, the spherical simplex 


13 
2 


is a spherical triangle P,P, 7. 
The quadratic form //, after being transformed, reads 
HH Gy? 749g %y +9 q © y $29.93 2g COSPy y $29,912 gi, COSP y +24, Jo iV COP, 


The opposite angle J/,, of the edge (or side) p,, now merely is 
the angle P, of the triangle. Denoting, for the present, the edges 
(or sides) by p,, Py, Ps» So that 


(eg 0 Tee 9 WS 


we have 
COR = —— COS Ti == —IC0Se 
and 
cos P, + cos P, cos P, ee ; 
COS Py, = C08 Py = = = =—- els, 
SUPE Spas V(1—r, ,?)(1—",,”) 


I= 1 — cos’ p,, — cos" p,, — cos” p,, + 2 cos p,, COS p,, COS P,, 
= 1 — cos’ p, — cos? p, — cos* p, + 2 cos p, cos p, COs ps. 
Putting further 
Pitptp=2s , P+P,+P,=28, 
we may reduce T to 
T= 4 sins . sin (s—p,) . sin (s—p,) . sin (s —p,) 
= 4 cos S. cos (S—P,) . cos (S—P,) . cos (S— =| 


0 TEA JER Gp Lee 
The relation 
ajay Biz 
= — = —_ a 


2 2H 


here involves 


Ons Of 
Be | by 5, Oss Jz Qs Sin® Pp, 
 — = = Sao Sete : 
In = 97 2B QE: 
Now 
a — 4 cos 8. cos (S—P,) . cos (S—P,) . cos (S—P,) 
e — . . . 4 
; GOs 1 i Tee 
hence 
sin? P 1 
i —e : x ’ 
13 2[—4cos S . cos(S—P,) . cos(S—P,) . cos (S—P,) ~~ q,? 
Putting 
— 4cos 8. cos (S—P,) . cos (S—P,) . cos (S—P,) = Q, 
we obtain 
ae ae 
io = 2 2 ’ 
whence 
sin P, 


ho 
u V2Qn,, 


Further we find, after reduction, 
Q = 1 — cos’ P, — cos? P, — cos? P, — 2 cos P, vos P, cos P,, 


consequently 
rae i Pa + 2 Toa Tig Ties 


Finally 
(RS one oe Oba qa" Osa Q° = 
= etek Pain? Phen Plein 873,N1s%ssQ 


Introducing the mean errors 7,, 9, and 9, of 2, 7, and a,, Which 


satisfy the equations 
& —— Pt een 
Ub 4h 9 Ye = hee 


yy = han ’ 


we find 
sin P; ; : 
ee ee) 


ni V2Q 


1 


Psa e Ie 


. 


E 


and 
Tes Tis Tie 


1 betel feat ih 9 723 ae 
=— ee — evel Je 
Geos. i eae 

ds, .05,.08,. 


Ps 
— 
(22)"2 1, 4,%,VQ 


157 


Mathematics. — “Combination of observations with and without 
conditions and determination of the weights of the unknown 
quantities, derived from mechanical principles. By Prof. M. J. 
van Uven. (Communicated by Prof. JAN pr Vaiss). 


(Communicated in the meeting of May 30, 1914). 


The theory of the combination of observations by the method oc 
Jeast squares has already been the object of numerous geometrical 
and mechanical illustrations. In the geometrical representations the 
leading part is usually played by vectors (L. von Scururka '), C. 
Ropricurz*)); the mechanical ones are taken partly from the theory 
of the ‘pedal barycentre” (Y. Vinuarceau *), M. p’Ocaene *) ), partly 
from the theory of elasticity (S. Finsrerwanper®) R. b’EmILIo‘), 
S. WeELnmIscH, PANTOFLICEK ’), F. J. W. Warrier’), M: WrsterGaarD *), 
G. ALBENGA ")). 

In the following paper we will try to develop a mechanical 
analogy of the solution of the equations furnished by observation, 
supposing that no conditions are added, as well as for the case 
that besides the approavimate equations of condition (called by us: 


1) L. von Scururka. Eine vectoranalytische Interpretation der Formeln der Aus- 
gleichungsrechnung nach der Methode der kleinsten Quadrate. Archiv der Math. u. 
Physik, 3. Reihe Bd. 21 (1913), p. 293. 

2) (C. Ropricurz. La compensacion de los Errores desde el punto de vista geo- 
metrico. Mexico, Soc. Cientif. “Antonio Alzate’, vol. 33 (1913—1914), p. 57. 

3) Y. Vimrarceau. Transformations de |’astronomie nautique. Comptes Rendus, 
1876 I, 531. 

4) M. p’Ocaene. Sur la détermination géométrique du point le plus probable donné 
par un systéme de droites non convergentes. Comptes Rendus, 1892 1, p. 1415. Journal 
de l’Ecole Polytechn Cah. 63 (1893), p. 1. 

5) S. Finsterwatper. Bemerkungen zur Analogie zwischen Aufgaben der Aus- 
eleichungsrechnung und solchen der Statik. Sitzungsber. der K. B. Akad. d. Wissensch. 
zu Miinchen, Bd. 33 (1903), p. 683. 

6) R. p’Emito. Illustrazioni geometriche e meccaniche del principio det minimi 
quadrati. Atti d. R. Instituto Veneto di scienze, lettre ed arti, T. 62 (1902—1903), 
p. 363, 

7) S. Wettscu. Fehlerausgleichung nach der Theorie des Gleichgewichts elasti- 
scher Systeme. Panroruicex. Fehlerausgleichung nach dem Prinzipe der kleinsten 
Deformationsarbeit. Oesterr. Wochenschrift f. d. 6ff. Baudienst, 1908, p. 425. 

8) F. J. W. Wutepte. Prof. Bryan’s mean rate of increase. A mechanical illustration. 
The mathematical Gazette, vol. 3 (1905), p. 173. 

%) M. WesterGaarp. Statisk Fejludjaevning. Nyt Tidsskrift for Matematik, B, T. 21 
(1910), pp. 1 and 25. 

10) G. Atpenca. Compensazione grafica con la figura di errore (Punti determinati 
per intersezione). Atti d. R. Acead. d. Se. di Torino, T. 47 (1912), p. 377. 


158 


“equations of observation”) also rgorous equations of condition 
are given. 

Moreover, in either of these cases also the weights of the unknown 
quantities will be derived from mechanical considerations. 

The method here developed is founded on the staties of a point 
acted upon by elastic forces and is in principle closely related to 
the procedure of the last-mentioned mathematicians. 

To obtain general results, we will operate with an arbitrary 
number CV) of unknown quantities or variables, which are consi- 
dered as coordinates in -dimensional space. In order to render the 
results more palpable, we shall, at the end, recapitulate them for 
the case of two variables. 

I. To determine the V unknown quantities 

ii iy. Zoe: ou « (UND) 
the » (approximate) equations of condition or equations of observation 
aja -+ by + o2+...4-m=0 (CS Oa) 
are given, with the weights g; resp. 

In the sums, frequently occurring in the sequel, we will denote 
by > a summation over the coordinates 2, Up poor OY Over the 
corresponding quantities (for inst. their coefficients @;,b;,¢;,...) and 
by | | a summation over the m equations of observation, thus over 
2 from 1) fom: 

Putting accordingly 

aj? + 6? +o? ... = Bia? 
and introducing 


aj bj Ci mM; 
oS VSae = Sat = Sas ANS bi see A 
we may write the equations of observation in the following form 
Vi=aet By tyet...+u=—0 G=1e 2) 
or 
V;=Zaje¢+ w= 0 (CSS thpo so): 


These equations have resp. the weights 
Pi=H > ai’. 

The equations V;=0 represent (V —1)-dimensional linear spaces; 
their normals have the direction cosines (aj, 3;, yi,-.-) resp. 

In consequence of the errors of observation, the approximate 
equations |; =O are incompatible; in other words: the n linear 
spaces 7;=0 do not meet in the same point. By substituting the 
coordinates w,y,z,... of an arbitrary point P in the expressions 


V;, the latter obtain the values v;, representing the distances of the 
point P to the spaces V;= 0. 

The distance from V;—=0O to P is to be considered as a vector 
»; with tensor v; and direction cosines a, Bi, yi,..- 

We now imagine a foree ¥; acting upon P (in V-dimensional 
space) in the direction of the normal »; (from P to V;=0) and the 
magnitude of which is proportional to the distance v; and a factor 
pi characteristic of the space V;. (The space V;=0, for instance, 
may be considered as the position of equilibrium of a space V;=7; 
passing through P by elastic flexion.) 

So the space V; acts upon P with the force 

$= — pity. 

All the spaces V;(¢=1,...n) combined consequently exert on P 

a resultant force, amounting to 
5 = [oi — [pal 

This resultant force depends on the position of the point P. 
Hence we have in .V-dimensional space a vector-field 5. determined 
by the above equation. 

Now the question to be answercd, is: at which point Pare these 
forces §; in equilibrium? For this point P we have 

=A") 
or 
lp pasi|i—20 

The “components” of this vector-equation in the directions of the 

axes are 


pore | 07 lor 87 0) perry 07s. 
Substituting for v; the expression V;= Sa;c-+- ui, we obtain 
[piai?] a + [piaiBi) y + [piaiyi] 2 +.-.-+ [pia cal === (l), 
[piGiai] « + [piBitly + [piBivile +--+ ipibiuil =. 
[piviei] « + [piyiBily + [piv le +--+ [piviu] = 9, 


. 


or by 
aj b; A Cj mj ; esas 
== ———_ , pi = = YS 8 SS SS EH HL MG =» 
VA OO V ai’ ar (ea 


[giai?] a + [giaibily + [giaic. ] 2 +--- + [gaimi]=0, 
[gibacle + [gibi*)y + [gible +.-- + [aibimiJ =O, 
[giccac |e + [gicrbily + [gia*]2 +--- + [giami] = 9, 


In this way the ‘normal equations” are found, 


160 . 


The force §;= — piti has the potential 
Ui= piv? =tpiVirs 
for 
: OU; OV; 
(Fi)x = — —— = — pi Vi —— = — pivia; ete. 
Ow Oa 


The whole potential therefore amounts to 
U=[Uil= 3 [pivi'). 
As the equation V;= Sa2-+4=0 has the weight p;, the 
mean error of weight 1 is determined by 


hence 


At the point P satisfying the normal equations the potential and 
consequently also €° isa minimum. The “weight” of the distance v; was 
pi- This weight may be determined a posteriori, if we know the 
influence of the space V; alone acting upon any point. We then 
have but to divide the amount /; of the force §; by x. 

II. In order to find the weights of the unknown quantities, we 
now remove the origin by translation to the point P, which satisfies 
the normal equations. 

Calling the minimum potential U/,, denoting the new coordinates 
by w',y',2',... and introducing 

V;'=aye' t+ Biy + ye +... aie’, 
we obtain 
lp? Va) 2 (Ey 20 

So U’ is the difference of potential existing between a point 
(v', y',2',...) and the minimum point P. 

The equation [p; V;"]=2U’ represents a quadratic (N — 1)- 
dimensiunal space &, closed (ellipsoidal) and having P as centre. 
This space is an equipotential space and at the same time the locus 
of the points of equal ¢. We shall call these spaces 2 briefly hyper- 
ellipsoids. The hyperellipsoids $2 are homothetic round P as centre 
of similitude. 

Introducing the principal axes as axes of the coordinates _X, Y, Z, ..., 
we obtain for £2 an equation of the form 

AX? BY? 2072 4... = 2107 

The components of § in the directions of the principal axes are 

found to be 


au" ? aU’ E du! a 
eS — dX =—_— AX, Fy =>— Pia —— Deh 7 — ry; === UC 
We may therefore attribute these components to attractive forces 
of the spaces ¥ = 0, Y=0, Z=—0,... (principal diametral spaces), 


which are perpendicular to these spaces and proportional to the 
“principal weights’ A, B,C,... 
For a point on the principal axis of X holds 
xe —— AX 1, oH yi — Ol 7 108 rete: 

Consequently the principal weight A may be determined by dividing 
the force at a point of the principal axis of X by the distance Y 
of that point to the principal diametral space Y = 0. To determine 
the weight of another direction !, only those points are required, at 
which the direction of the force coincides with the direction |, i.e. 
the points the normals of which to the hyperellipsoids $2 have the 
direction 1. When dividing the amount of the force existing at such 
a point Q by the distance of the tangent space of Q to the centre 
P, the quotient found is equal to the weight of the given direction. 

So, in order to determine the weight g, of the direction of the 
original z’-axis (or of the w-axis), we only have to turn back to the 
coordinate system w,y7/',2',..., relatively to which the equipotential 
spaces have the equation 

WA 40 

For a point Q(a’,y’,z',...) at which the normal to the equipotential 
space, passing through Q, is parallel to the w'-axis (or to the x-axis), 
we have 

Ffys—g0' , Fy=0 , Fy=0, ete 


or 
so pe our Ou! 
apr = 9 , eae : ape ete, 
hence 
[pia Vi] == gee! , [pir Vi'}=0 , [piyiVi'] =, ete, 
or 
Lpiai*] a + [piaisil y' + [piaivi] 2! +... = goa’, 
[piBia:]e' + [piBi7ly + lpi Bivile' +-...=0, 
[piy.ai |e’ + [piviBily' + (piyZ)]e' +... 9, 
or 


y! 
Dpa 


: 1 : eH 
[pia |— + [piaibi] — + [piaiys] —-+...—1=0, 
Ju 4 Jat 


! 


; | i zZ ’ 
[pi Bias] — + [pi Bi") if + [piBiye]—t+.-..+90=9, 
Ja Jad Jat 


It ea 
[piyees] — -[piviBi]— + [pivi*] — +--- -0=9, 


Ix Jar Ja 


or 
] y! 2! 
Jgiai?] 7 all le [gia; b; | ——1 |= laiaic | es +...— 1 == (0) 
Ix Jar Jak 
1 < Of Zz 
lgbier] + [9 8i*] — +. [gi bit] — 2 =-F 0 = 0; 
Ox et Dyk 
1 y' ber 2 : 
[gicia;| == [eieib; = =— [gier=]) —— + - - = 0; 
Ix Jat Jat 
Yo aes 4 ag ble 
So — is apparently found as the first unknown quantity in the 
De 


“modified” normal equations, modified in this way, that the constant 
terms are replaced by — 1,0,0,... resp. 

Considering U (e.q. U;) as an (N + 1)" coordinate perpendicular 
to the N-dimensional space (v7, v, z,...), the equation 

Vii 20; 
represents a quadratic space of NV dimensions, built up of 0 (N—1)- 
dimensional linear generator-spaces, all parallel to (V;=0, U=0), 
the intersections of which with the planes perpendicular to (V;=0, 
U7=0) are congruent parabolae. The parameter of these congruent 
parabolae is —. 
pi 
The quadratic space pi Vi? =2U; will briefly be called a parabolic 


eee ; il 
cylindric space with parameter —. 
su Di 
The equation 


| pi V2) 2 U 
represents a quadratic space W of N dimensions, the centre of which 
is at (7 =o, and the intersections of which with the V-dimensional 
spaces U = const. are hyperellipsoids 2. Thus YW is the extension 
of the elliptic paraboloid. 

The point 7 of WY with minimum JU (U,), and hence closest to 
(7=0, which is called the swmmit of ¥% is projected on U=O 
in the point P, satisfying the normal equations. 

By displacing the system of coordinate axes (w, y, 2,...,U) (by 
translation) from O to 7, ¥ obtains the equation 

[pi V;"] = 2 U'=2(U—D)). 


By constructing the enveloping cylindric space, the vertex of which 


163 


coincides with the set of points of the space «—O at infinity, thus 
the tangent cylindric space, the generator-spaces of which are parallel 
to the z-axis, we find for this cylindric space the equation 


Onatha ——ay life 


Ree : 
Its parameter is —, or the reciprocal value of the weight of the 
Gx 
direction «. 


Ill. We now suppose, that the variables w, y,2,... must at the 
same time satisfy the following » rigorous equations of condition 
Day ee) 0 (Gisaa5, 2) 
Then the point P is constrained to the common (V—»)-dimensional 
space ® of intersection of the »(N—1)-dimensional spaces ®;. 
Now the point P, subjected to the elastic forces §;, is in equi- 
librium, when the resultant 4 = [6;| is perpendicular to ®. 
Let the normal at P to #; have the direction cosines 
O®; OP; 0’; 
Ow Oy Oz 


a! J 


eae a Se tc 
(98 ee 0@;\? ca (0D; \; ie 
SS > 
v>(5') a CG) v3(%) 


The normals at P to the spaces #; form a linear v-dimensional 
space. In this space % must lie, which means: § can be resolved 
in the directions of these normals, the wnit-vectors of which will be 
denoted by w 

So we have 


a 
— 


5 = [9 wy] 
where | ]' signifies the summation over j from 14 to ». 
The components of this vector-equation are 
Lpivias |] + [99 as’! =0, [pe riBi] + Lay B=, [piri ye] + [qi vi']'=09, ete. 
or 
[piai*] x + [piarBily + {pieivi] = +--+. + [piaiui] + [gj ey] = 0 
[piBiec] @ + [pibi*] y + [peBivi] 2 4- ©. - + [piBiwi] + lay 8;'T = 9, 
[piyi ag] @ +- pees Ny Yet Piva lee seer ‘ [piyier] + [aj v5) =, 


Q 


Putine 
a ee? ie ae a, 
G=UVV= » (y=1,..>) 


Ow , 
we may write the above equations in the form 
, OD; 
Ow 


=20) 


[giai*) @ + [giaidi]-y + [aiaic le 4+... + [giaimi] + [qi 


164 


0D; , 
[qi bai) @ + [oi bi*] y + [oi dici] 2 4-6 <. =E [ai bimi | + lay >, l=05 
y 
0; _, 
[meres ]@ + [oerbi]y + [oe] 2 +... + oem) + [y' 7 Y=0, 


These N equations serve, together with the » conditions ®; =0, to 
determine the NV variables 2, y, 2,... and the vy auxiliary quantities q;’- 

Now the solution of the problem is not represented by the centre 
of the hyperellipsoids £2, but by the point, in which the intersection 
space ® (space of conditions) is touched by an individual of the set 
of the hyperellipsoids 2. 

The analytieal treatment of the problem is simplified by taking 
the coordinates so small, that in the expressions ®; homogeneous 
linear forms suffice. The geometrical meaning of this is that a new 
origin O' (vy, Yo, Zo, --) IS Chosen in the space of conditions ® near 
the probable position of the required point. So the spaces ®; are 
replaced by their tangent spaces /;, and the space of conditions by 
its tangent space R&R of N—vr dimensions, intersection of the tangent 
spaces Lj. 

Denoting the coordinates obtained by translation to O’ by §, 9, §, «., 
so that e—.w2,+6,... and putting 
ae, + Biy, + Yiz%) + aah , axe, + by, + cz, +... + mj = mi; 
we find 
2U =[pilaiw + iy + yi» + wi] = [pais + Bin + iS + + HH) 

putting 
aE + Bin + iS 4-... gi Vi, 
20i= [pi Vi). 
The equations #; (x,y,z...) = 0 may now be written: 


(Pbjn Odd) (Day 
Ds (a5) Yurzo.- - | —— 5 ' ) ae C+...)/+..S0 


Ow 
or, since O” is assumed in ®; =O, and higher powers of §, 7, &... 
are to be neglected, 


OD; OD; OD; io : 
Eee be 02 (y= ee) 
Ow Oy 


02 
or 
W,=a;§+86;n+y7/S$4+...=2a;5=0. (j=1,..-»). 


So the normal equations appear in the following form 


[viae?) § + [eae br] + (yeaie |S +.» + [gcaimi] + [ar oy!) = 9, 
[yi bias | § + [gobi] my + [ue bier]$ + -- + [ge dime] + Lay 2s! =% 


165 


lgccraz] § + [gecebs] y 4 Lore?) $+. + [oiceme] + ony lk 05 


IV. To determine the weights of the directions a, y, z,..., we 
again begin by shifting the origin (by translation) from QO’ to the 
point P, satisfying the normal equations and |W’; = 0. 

a : . 7 

Calling U, 
potential relatively to P, &’,9)’,6’,... the coordinates with respect 
to P, and putting finally 


the potential in P, (7—U,=U" the difference of 


as + Big py Se. vil, a St Bin! + yi G+... = Wy 

we find 
20) lp Va 2h; Wei 

This equation represents the set of equipotential spaces 2. U/’=0 
furnishes the byperellipsoid 2, touching ® (or 7?) in P. 

Now those points must be found at which the force can only be 
resolved into an (inactive) component perpendicular to FR and a 
component parallel to the «-axis. 

For such a point we have 


aU ‘i 
carts Feta [yee] — ges), 
al OU! r nr 
EE — a on et 0, 
U/ 
eu! : 
ee aie Cee Stare 
or 
Lpi Vir ac) -— [qpe3') = — [rye;']' + oe8', 
[pi Vi Bil — (q98;') = — [585], 


[pi Vi! vil — lays) = — Ura, 


or putting 
i) = == 8 
[pias Vi'] + Lsjery''=a8', [pi 8! Vi'] + [553;'=0, [prvi Vi'l+1s;7;'I'= 0, ete. 
whence = 
Lpiai* |S + [pias Bil a! + [pieivi] § + ~~~ + [sjey'|’ = ge8', 
[pieiai]s’ + Lpeei*) a! + [reir 1S + -.- + [s78;']' = 9, 
[piy es + pivibi)a + [pixels 4 T=9, 


oo ae ey 
or 


Proceedings Royal Acad. Amsterdam. Vol. XVIL 


166 


Is 9s 


Ube 7 q eee 
[aiai?] - + [giajb; | - i + [gja; a See es) 
dé = 


1 , | oS) $j 
[9% ba; }— + [9: b; 7] = + a be; | SS Roo oS | [tj + 0 == (i). 
gz Grs zs q | 


Js JSS 


1 / 2 S 7) " 
lo:ciai |] — + [oie b; | oad + lai c*] Sqn 050 Sr 6 9A 10 ==10" 
5 : 


the conditions 


' 1 ' 7] ! o . 
aj +f 85) = ee ae (Gj = 5 5.0.9))s 
gs ges 98 


also being satisfied. 
From the above NV -+ » equations with the V unknown quantities 


1 9 C sos wy 1 
.—=,——,... and the rv unknown quantities — , — can be solved. 
ge 98) eS 9:5 9 


The method of solution of Hansen is found again by introducing 


SSS an <7 
Gs $j ! 
es SS) 
S a] et) 
i) JES 
<! 1 ! ' 
s qj 
= — A == iB ; 3 = G& ; 
9S GE JES ges 
whence 
k; Sajé' 
=-= — = Taj A (G1 n) 
gi JES 


Then the modified normal equations furnish 
[9ia;?] A + [giaibi] B+ [gait] C + ...+ [kj'a,;'|’ =1, 
[ai bia: | A + [oibi? |] B+ lai bie] C+... 4+ [k;'8;'] == (()): 
[9iccai] A + [obi] B+ [gic?|] C 4-..-+ Tew) =9, 


or 
[g:ai(2a; A)] + [egal als lig: b;{ 2a; A)| + [4;'3; ]=9, 
[gi ¢i (a; A)] + [é;'y;'T =) eiGe 
or 


[kia;] + [ej'o,'! = 1, [eib:] + [4,'8,'|' =, [hier] 4 [4)'7;'' =O, ete., 
and the (rigorous) equations of condition run 


= a; A— 0 (Gi eee) 
From the set of equations 
: Bi wae ee 
=q, A= — (ee) 
Ch 
>), A —— 10) (== ono), 


[cag Ay ey" |'=1 , [he bs 4 [4y'8;''=0 5 [Ai ci JH-14;'y;']=0 , ete. (NV in number) 
the .V variables A,B, C,..., the m unknown quantities %; and the 


yr auxiliary quantities /;' can now be solved. 


167 


The weight of x is thus defined by 
1 
Ia — 9 =S = 


A 


It may also be found by the following ealeulation 
ke? 
a = [hia A] = ZA [hia;] = A [hia;] + B [kbs] + C [hier | 4 
=A— A [ka — B[AB;] — C [h'7;J —... 
ll 
= Al = Gea) = Se 


95 
so that g, is also determined by 


7a 

EA 

By considering the quantity U as (V + 1)" coordinate perpendi- 
cular to the N-dimensional space (7, y,z,...), the equation 

[p: Vi'?] — 2 [g; W;') = 20" 
represents the quadratic space ”. The origin of the coordinates 
§',7/,0,..U' now lies at the point S, the projection of which on 
U'=— U,(U=D) is the required point. Now this point S is not 
the summit of ¥. 

The linear space of conditions R of NM —» dimensions is now 
joined to the point U” = @ by an (NV —v- 1)-dimensional space R,, 
which passes through S and intersects the quadratic space ¥ in a 

1 
also has its centre in U’ =o, but is of fewer dimensions, viz. 
N + (N—-++1) — (N-++-1) = N —v. The quadratic space ¥, has 
its summit in S. 
We now have to determine the points Q in ¥,, at which the 


quadratic space ”, having the same character as Y, in that it 


((v-+-1)-dimensional) spaces of normals are parallel to the a-axis. In 
such a point Q ¥, is also enveloped by a parabolic cylindrie space, 
the generator-spaces of which are parallel to the a-axis, and which 
therefore has an equation of the form 

gx §? = 2. U'. 


1 


Ya 


Its parameter is 


ao 
In other words: — is the parameter of the parabolie cylindric 
Ya 


space, which has its generator-spaces parallel to the a-axis and 
envelops the quadratic space ¥, . 


V. We conclude this paper with a short summary of the results 
for the ease of two variables w and y. 
12* 


168 


The equations of observation are represented by the straight lines 
Vi;=aje + By + w=O (weight pi) @=1,...n). 
The point P(, y) is subjected to the force 
6 = [di] = — [piri] 
in which », represents, in amount and direction, the distance of the 
line V;=0 to the point P. 
The point P remains at rest, if its coordinates satisfy the equations 
[pias] @ + [piaiBily + Lriecui] = 0, 
[piBiai]@ + [piBitly + [piBier] = 0. 
Denoting here the potential U7 by 2, we obtain 
[pi(ace + Biy + wi)?] = 22. 
This equation represents an elliptic paraboloid ¥, being the sum- 
surface of the parabolic cylinders 
pilare + Bry + fy)? = 2z;, 
which have the plan z—O as summit-tangent-plane along the gene- 
rator ae + By --+ wi 0, z= 0, and which are obtained by trans- 
lating the parabola 


lying in the normal plane of Vi= «je + 3:y 4+- a= 9, perpendicularly 
to V;=0. The parameter of this parabola is ok 
i 

The summit 7’ of the elliptic paraboloid ¥ ({p; V,*] = 22) is pro- 
jected on z—0O into the point P, satisfying the normal equations. 

By constructing the tangent cylinder, the vertex of which lies 
upon the «-axis at infinity, we obtain a parabolic cylinder, the 
perpendicular transverse section of which has a parameter equal to 
the reciprocal value of the weight g, of the variable a. 

There being only two variables, only one (rigorous) equation of 
condition &(v,y)—=0O may be added; (x,y) =O represents the 
curve to which the point ? is constrained. 

We now have to determine that particular ellipse of the homothetic 
set [p; Vi?]=const., which touches the curve @. The point of 
contact is the point P required. 

In #, near the probable position of P, the new origin O% is 
taken. We have thus only to operate with linear functions of the 
coordinates. So we really replace ® by its tangent R at P. 

The elliptic paraboloid 7 is cut by the vertical of P in the 
point S. The vertical plane &,, which intersects z=0O along R, 
pierces the paraboloid 4 along the parabola ’,, having Sas summit. 

We now construct the cylinder having its vertex at the point 


169 


at infinity of the «z-axis and having the parabola ¥, as directrix 
(ie.: enveloping the parabola ,). The parameter (of the perpen- 
dicular transverse section) of this cylinder is the reciprocal value 
of the weight g, of the variable z. 

The equipotential lines in 2=0O are the homothetic ellipses 
[pi Vi? | =const. Such an ellipse is the locus of the points of equal «. 

When the (rigorous) equation of condition is: «= ceonst.. the 
parabola , is parallel to the plane «=O. The tangent cylinder is 
then infinitely narrow ; its parameter is 0, the weight of « is infinite. 


Chemistry. — “Kquilibria in ternary systems. XVI. By Prof. F. 
A. H. ScHREINEMAKERS. 


(Communicated in the meeting of May 30, 1914). 


Now we shall consider the case that the vapour contains two 
components. 

We assume that of the components 4, 6, and C only the com- 
ponent 6 is exceedingly little volatile, so that practically we may 
say that the vapour consists only of A and C. This is for instance 
the case when B is a salt, which is not volatile, and when 4 and 
C are solvents, as water, alcohol, ete. 

Theoretically the vapour consists only of A+ £-+ C; herein the 
quantity of B is however exceedingly small in comparison with the 
quantity of A and C, so that the vapour consists practically totally 
of A and C. 

When, however, we consider complexes in the immediate vicinity 
of the point 5, the relations become otherwise. The solid or liquid 
substance has viz. always a vapour-pressure, although this is some- 
times immeasurably small; therefore, a vapour exists however, 
When we now take a 


Y 


which consists only of 4, without A and C. 
liquid or a complex in the immediate vicinity of point B, the 
quantity of 4 in the vapour is, then still also large and is not to be 
neglected in comparison with that of A and C. 

Consequently, when we consider equilibria, not situated in the 
vicinity of point 4, then we may assume that the vapour consists 
only of A and C; when these equilibria are situated, however, in 
the immediate vicinity of point 4, we must also take into consider- 
ation the volatility of 45 and we must consider the vapour as ternary. 

When we consider only the occurrence of liquid and gas, then, 
as we have formerly seen, three regions may occur, viz. the gas- 
region, the liquid-region and the region L—G. This last region is 


170 


separated by the liquid-curve from the liquid-region and by the 
vapourcurve from the vapour-region. As long as the liquideurve is 
not situated in the vicinity of point 6, the corresponding vapour- 
curve will be situated in the immediate vicinity of the side AC. 
Consequently the vapour-region is exceedingly small and is reduced 
just as the vapourcurve, practically to a part of — or to the whole 
side AC. Therefore we shall call this vapoureurve the straight 
vapourline of the region £— G in the following. Consequently we 
distinguish within the triangle practically only two regions, which 
are separated by the liquideurve, viz. the liquidregion and the region 
L—G:; the first reaches to the point B, the latter to the side AC. 
The conjugation-lines liquid-gas end, therefore, all practically on the 
side AC. 

When the liquideurve comes, however, in the immediate vicinity 
of point B, so that there are liquids, which contain only exceedingly 
little A and C, then the quantity of 46 in the corresponding vapours 
will no more be negligible with respect to A and C. The vapour- 
curve will then also be situated further from the side AC, so that 
also the vapour-region becomes larger. At sufficient decrease of 
pressure or increase of temperature the vapour-region will cover 
even the entire component-triangle. In that case we must, therefore, 
certainly distinguish between the three regions, of which the movement, 
occurrence and disappearance have been treated already previously. 


In order to deduce the equilibrium #'+ L+G, we may act now 
in the same way as we did before for a ternary vapour. We dis- 
tinguish the following cases. 

1. The solid substance is a ternary compound. 

2. The solid substance is a binary compound of two volatile 
components. 


3. The solid substance is a binary compound of one volatile and 
one non-volatile component. 


4. The solid substance is one of the components. 


1. We consider firstly the case sub 1, viz. that the solid substance 
is a ternary compound; this is for instance the case with the 
compound Fe,Cl, . 2HCl.12H,0. 

Now we imagine for instance in fig. 7, 11, 12, or 13 (I) the 
component-triangle ABC to be drawn in such a way that the point 
F is situated within this triangle. Curve Mm can then again 
represent the saturationcurve under its own vapourpressure of F, 


val 


the corresponding vapourcurve J/,;m, is then, however, no more a 
curve situated within the triangle 46C, but it becomes a straight 
line, which is situated on one of the sides of the triangle. We shall 
call this line the straight vapourline of the compound /. When A 
and C' are the two volatile components, then this straight vapourline 
is situated on the side AC. As not a single liquid of curve J/m can 
be in equilibrium with a vapour, which consists of pure A or of 
pure (C, the points A and C’' can never be situated on the straight 
vapourline. From this foilows: the straight vapourline of the ternary 
compound /#’ covers only partly the side AC and in such a way 
that it covers neither A nor Bb. 

2. The solid substance is a binary compound, of two volatile 
components. We take a binary compound F' of B and C (tig. 1) 
so that 5 and C' now represent the two volatile components and A 
the non-volatile component. 

In order to deduce the saturationeurve under its own vapour- 
pressure we may act again in the same way as we did before 
for the general case. For this we take a definite temperature 7’ and 
a pressure ? in such a way that no vapour can be formed and the 
isotherm consists only of the saturationcurve of /°. This is represented 
in fig. 1 by pq. 

At decrease of P the region L—G occurs; such a region is 
represented in fig. 1 by Cdee, with the liquid-curve de and the 
straight vapourline Ce,. The liquid’ e is in equilibrium with the 
vapour é,, the liquid @ with the vapour C and with each liquid of 
eurve ed a definite vapour of the straight vapourline Ce, is in 
equilibrium. 

We may distinguish three cases with respect to the occurrence 
of this region L—G. 

a. In the equilibrium L—G of the binary system BC a point of 
maximum-pressure occurs. The heterogeneous region L—G arises in 
a point of the side BC. 

b. In the equilibrium L—G of the binary system BC a point of 
minimum-pressure occurs; one heterogeneous region arises in 2 and 
one in C, which come together at decrease of P in a point of BC. 

ce. In the equilibrium L—G of the binary system SC’ neither a 
point of maximum- nor a point of minimumpressure occurs; the 
heterogeneous region arises in / or in C. 


Here we consider only the last case and we assume in this case 
that Cis more volatile than B; after this the reader can easily 


deduce the two other cases. At 
decrease of P the heterogeneous 
region arises, therefore, in the angu- 
lav point C’ (fig. 1) and it expands, 
while curve pg changes of course 
its form and position, over the 
triangle. Under a definite pressure 
the terminatingpoint e of the liquid- 
curve coincides with the termina- 
tingpoint p of the saturationcurve, 
under a definite other pressure e 
coincides with ¢. 

When e coincides with g, we 
may imagine in fig. 1 that the 
liquideurve is represented by qq’, 
d or by gqq',; in the latter case it 
intersects the curve qp, in the first 


case it is situated outside this curve. When e coincides with p, we 
may imagine that the liquideurve is represented either by p/ (fig. 1) 
or by a curve, not drawn in the figure, which intersects pq. Now 
we shall examine which of these cases may occur. 

To the equilibrium between a ternary liquid w, y, 1—a—y, and 
a binary vapour y,, 1—y, the conditions are true: 


ee 5 fans, : 
et! an Tin (y—y,) Ox = 4, anc Oy Oy, So te eS eee ) 


Let us firstly consider the region L—G in the immediate vicinity 
of the point C. As x,y, and y, are then infinitely small, we put: 


Z=U+RT2rlogx+ RT y logy and Z,= U,+ RT y, log y, 


The two conditions (1) pass then into: 


OU OU OU 
U—#«# — —y— — U, +4, SSR (@ + y—y,)=0 . (2) 
av Oy Oy, 
OU we OU, ; ’ 
— + RY logy=—+ RT logy, . . . . . (8) 
Oy Oy, 


Under a pressure Pe the region Z-G in fig. 1 consists only of 
the point C, and, therefore, «=0, y=O and y,=0O; then the 
unary equilibriam: liquid C+ vapour C oceurs. This is fixed by 
LZ=fZ, 011 U= U,, wherein: 2 = 057 = 0sande7y)— 10: 

Let in fig. 1 the region Cdee, make its appearance under a pres- 
sure Po + dP; the points e,, e, and d are then situated in the imme- 


Lio 


diate vicinity of C; now we equate «= §, y = and y, = 1. From 
(3) follows: 

1 = ae cee a et Ae fe (4) 
wherein AK is a constant fixed by (8). When we assume, as 
in fig. 1, that Cis more volatile than 6, the point ¢, is situated 
between C and e and “J is, therefore, smaller than 1. 

Nowe we equates ()) == Po = dP vai ey — 7) andy, = 7. : 
as in the point C U= U, is satisfied, it follows, that: 
—RT[E+ y= y,) +[V—V,|dP=0 
or 


E41 (—K) —— dPighs Seema) am (5) 

In the immediate vicinity of the angular point C (fig. 1) curve ed is, 
therefore, a straight small line. We find from (5) for the length of 
the parts Cd and Ce: 

V,--V : Via 
——— dP and Ce= — —————dP. . . . (6) 

RI Ri (ea) 

As V,—V >0 and 1—K > 0, it follows from (6) that Cd and Ce 
are positive, when dP is negative. At decrease of pressure curve ed 
shifts therefore, within the triangle. From (6) follows :Cd: Ce=(1—A);: 
imoreeas: 1 — 7 — Coan Ce: we. find: Cd = eex 

In order to examine the lquideurves going through the points 
p and q (fig. 1) in the vicinity of these points, we put in (1): 


C= — 


Mie) ( UB Bed RI LRRD oa tc RB Stace oun WL) 
we then find: 
U—a ee —(y—y ee —RT«e—Z, =0 wae eaeies . (8) 
Ow Matar : Oy Oy: 


For the liquideurve of the region L-G we find from this: 
[er + (y—y,)s + RT] de + [as + (y—y,)t]dy=0 . . (9) 
For the direction of this liquideurve in its end on the side BC 

(therefore «= 0) we find: 
dy y—y_) s-— RI 
oh a Uae (10) 
da (y—y,) t 
When we call g the angle, which this tangent forms with the 
side BC (taken in the direction from 4 towards C), we have, when 
we imagine the componenttriangle rectangular in C: 
(y-—y,) ¢ 
Ch. ———— =5 
(y—y,)8 + RI 


| 


(11) 


174 


For the saturationcurve under a constant pressure of /’, consequently 
for curve pq, we find: 
OZ 0Z 


Z—x - (8—y = (Ge R age 0 (file 
Z—a— + (8 Day oa (12) 


or after substitution of the value of Z from (7): 
[er + (y—B)s + RT] dx + [xs + (y—p)t]dy=0 . . (183) 


When we call wy the angle which forms the tangent in p or q 
with the side BC (taken in the direction from 8B towards C, 
we tind; 

gs EE 
(y—B) s+ RI 

Let us now consider these two tangents in the point p of fig. 1. 
In this point y—3< 0 and y—y, > 0. 

The denominators of (11) and (14) bave, therefore, either opposite 
sign or they are both positive, so that we may distinguish three 
cases. In each of these cases we find y < w; the liquidcurve of the 
region /.-G and the saturationcurve of / under a constant pressure 
are, therefore, situated in the vicinity of point p with respect to 
one another in the same way as the curves pf and pq in fig. 1. 

Curve pf can also no more intersect curve pg in its further 
course; we may see this also in the following way. 

At decrease of P the two curves must touch one another under 
a definite pressure P;, somewhere in a point / within the component- 
triangle; therefore imagining the liquideurve of this pressure P, 
to be represented by ed (fig. 1), we must imagine ed to be drawn 


2 z ; : dy 
in such a Way that it touches pg in h. For this point nh trom (9) 
ax 


dy 
must be equal to ;_ from (13); then holds: 
aw 


ar + (y—y)s + RT ar + (y—3)s + RT 15 
ast(y—y)t ws + (y—pa)e . 20a 


or 
a) veiw oo sg (1G) 


As y, indicates the vapour conjugated with liquid 4, (16) means: 
the liquid-curve of the region L—G and the saturationcurve under 
a constant pressure of /# touch one another in a point 4, when the 
vapour belonging to this liquid / is represented by the point /. 

As all vapours belonging to curve ed (fig. 1) are represented by 


175 


Ce,, and consequently no vapour exists of the composition /’, the 
curves ed and PY therefore, cannot touch one another. 

Let us now consider the tangents to the liquid-eurve and to the 
saturationcurve under a constant pressure in the point q (fig. 1); 
as the vapour, belonging to this liquid, may be represented either 
by a point q, situated between gq and F or by a point qg, between 
F and C, we must distinguish two cases. 

When the vapour is represented by g,, then we have y— 7 >0 
and y— y, >0. As y—/??>y-— y,, the denominators of (11) 
and (14) have either the same sign or the denominator of (11) is 
positive, while that of (14) is negative. In each of these three cases 
we find g<ywy; the liquid-curve of the region L—G and _ the 
saturationcurve under a constant pressure of /’are, therefore, situated 
in the vicinity of point g with respect to one another as the curves 
gp and qq',. 

When the vapour corresponding with lquid g is represented by 
q,, then y— /? <0 and y —y, > 0; in absolute value (y—/?)s is 
always smaller than (7 — y,)s. The denominators of (11) and (14) 
have, therefore, either the same sign or the denominator of (11) is 
negative, while that of (14) is positive. In each of these three cases 
we find ~ >y; the liquid-curve of the region L—G and the 
saturationcurve under a constant pressure of /’ are, therefore, situated 
in the vicinity of point q with respect to one another as the curves 
gp and qq’,- 

With the aid of the preceding considerations we may easily deduce 
now the saturationcurves under their own vapour-pressure of /’; 
for this we shall assume that the solid substance melts with increase 
of volume. We distinguish three cases. 


1. The temperature is lower than the point of maximum-subli- 
mation 7x of the binary substance /. 

In a similar way as we have deduced the general case fig. 11 (I) 
we now find with the aid of fig. 1 for the saturationcurve under 
its Own vapourpressure a diagram as is drawn in fig. 2; in this 
figure a part only of the componenttriangle is drawn. Curve 
hacmbn is the saturationcurve under its own vapourpressure, 
h,a,¢c, FP, b,n, is the corresponding straight vapourline. In_ this 
figure are indicated the equilibria: #74 Ln + Gy,, M+ La + Ga; 
FLEL+ Ga, P+ In+ Ge F+ y+ Gy, and F+ L, +Gn,; Ln 
and £, ave binary liquids. As we have assumed that the temperature 


d 


is lower than the point of maximum-sublimation 7%, of the solid 


176 


substance #’, the vapour m, must be situated 
between #’ and x. Consequently we have 
here the case that the vapour, corresponding 
in fig. 1 with the liquid g, is represented 
by q,; the liquid-curve of the region L—G 
going through the point qg can, therefore, 
be represented by qq,’ (fig. 1). It follows 
from this position of gq,’ that on further 
decrease of pressure the liquideurve of the 
region L—G must touch curve pg ina 
point m (fig. 1); in fig. 2 this point of 
contact is also represented by m. Previously 
we have seen that the vapour corresponding 
with such a point of contact has the com- 
position #’; in fig. 2 m and F are joined 
for this reason by a conjugation-line. 

Fig. 2. It follows from this deduction that the 


pressure is a minimum in the point m of fig. 2 and increases from 
m in the direction of the arrows, consequently towards n and h. 
Further it is evident that the vapourpressure in / is higher than in 7. 


2. The temperature is higher than the point of maximum subli- 
mation 7’~ and lower than the minimum-meltingpoint 7p of the 
substanee F. 

In a similar way as we have deduced the general case fig. 7 (I), 
we now tind with the aid of fig. 1 a diagram as fig. 3. Curve 
hachun is the saturationcurve under its 
own vapour-pressure, /, a,c, 6,1, 1s the 
corresponding straight vapour-line. As 
we have assumed that the temperature 
is higher than 7’_ but lower than 7'p, 
F must, as in fig. 3, be situated between 
n and n,. Therefore, here we have the 
case that the vapour, corresponding in 
fig. 1 with the liquid g, is represented 
by qg,; the liquid-curve of the region 
IL—G going through the point g may, 
therefore, be represented by qq‘. (tig. 1). 
It follows from this position of qq, that 
on further decrease of pressure the liquid- 
curve of the region L—G no more 


intersects curve PY: 


177 


From this deduction it follows that the pressure increases along 
curve /im in the direction of the arrows, therefore, from 2 towards 
h and that on this curve im neither a point of maximum- nor a 
point of minimumpressure occurs. 


3. The temperature is higher than the minimum-meltingpoint 7’ 
and lower than the point of maximum-temperature 777 of the binary 
equilibrium #’+ 1 -+ G. 

In a similar way as we have 
deduced the general case fig. 12 (1) 
we now find for the saturationcurve 
nnder its Own vapour-pressure an 
exphased curve, in fig. 4 a similar 
curve is represented by the curve 
hn indicated by 5; the pressure in- 
creases in the direction of the arrow, 
consequently from n towards h. 


In fig. 4 the saturationcurves 
under their own vapour-pressure of 
F are drawn for several tempera- 
tures (7,—T,). When we take 7, 
and 7, lower than 7x, then a 
point of minimum-pressure must 
occur on the curves, indicated by 
1 and 2. When we take 7’, between 
Tx and Ty and 7, between 7'x 
and 7’'y7, then the saturationcurves Fig. 4. 


under their own vapourpressure have a position as the curves /2 
indicated by 4 and 5, on which no point of minimumpressure 
occurs. At 77 the saturationcurve disappears in a point A and 
the corresponding straight vapourline im a point //, (not drawn 
in the figure). 

On the saturationcurve of the temperatures 7’, and 7’, we find 
a point of minimum-pressure m, this pomt has disappeared on the 
saturationcurve of the temperature 7’, ; between these two temperatures 
we consequently find a temperature 7’, at which the point m coin- 
cides with the terminating point 2 of the saturationcurve under its 
own vapourpressure. As the vapour belonging to a point of minimum- 
pressure has always the composition /’, this case occurs when the 
liquid 2 can be in equilibrium with a vapour /” As then the binary 
equilibrium /’-+ £-++ vapour /# can occur this temperature 7%, 


: 178 


consequently is the maximumtemperature of sublimation 7x of the 
substanee /’. 


Now we will deduce in another way the saturationcurves under 
their own vapour pressure of /. The conditions of equilibrium are: 


WA OZ OZ 07 07 
a -— == fi - == 5 i =p} ah —C eS eres é iy; 
ae (y—/?) hoo: .—(y,—/?) Sg ae ae (17) 


These conditions follow also from the equations 1 (II) when we 
equate herein @ =O and «, =O and when we consider 7, as inde- 
pendent of «,. We put 

Z—= U- RT ailogm 0.) ee 


The three conditions (17) pass then into: 


U—a« ae — (y—/?) gu = tala 5 =O cee (19) 
Ow : Oy i 
Z,—(y 7) Oe eee Sock) Ls her 
a eae OD 
nA 


From this follows: 


far + (y—/?)s + RT| da + [as + (y—)¢#] i — 


ay av 
— | V—e on = (y—/?) rm =< ie. ers as ee (22) 
x Yy 
F hes , OV, ‘ : 
(y,—/*) t, dy, =| Vi\—(y.—") a =—wl|dP . . 7 4(23) 
; i 


av. av. 
sdx + tdy—t, dy, = a ea en P . - ae (24) 
dy, dy 


With the aid of (23) we may also write tor (24,: 


ee OV 
(y,— 7) sdx + (y,—)tdy = i ; (y,—,;9) a oar (25) 
dy 


so that for the relation between da, dy, dy,, and dP we shall consider 
the equations (22), 23), and (25). 

In order to examine if a point of maximum- or of minimum- 
pressure is possible on the saturationcurve under its Own vapour- 
pressure, we take (23). From this follows ¢? =O when 

Gia 0 ss on Ae 

In order to examine if the pressure for this point is a maximum 
or a minimum, we develop (20) further into a series: when we 
equate herein y, = /7, we find: 


Wes) 


1 
(V,—2) Oe == = t dy,’ 5h FA nee ach Sere ne (27) 


< 


As V,—v and ¢, are both positive, it is apparent that the pressure 
is a minimum. In accordance with our previous considerations (see 
fig. 2) we find therefore: on the saturationcurve under its own 
vapourpressure of the solid substance /’ the pressure is a minimum 
in a point m, when the vapour corresponding with this liquid has 
the composition 

In order to examine the change of pressure along the saturation- 
curve in the vicinity of its extreme ends / and 7 (fig. 2, 3, and 4) 
we equate «=O; from (22) and (25) we then obtain: 


T 


oy 
[(y—-/?)s + RT] du + (y —B) t dy = [V—-(y—/?) ai —ydP . . (28) 


= 


Oy 
(y,—/?) sdx + (y,—B) t dy = [V,—(y.—,*) ar vyjdP. . (29) 


From this follows : 
(y, —/?) RTdx = [(y,—/?) V + (@—y) V, + Y¥—y,) ey] dP. (80) 
When AJ, is the change of volume, which occurs when between 
the three phases of the binary equilibrium #’'+ 4+ G a reaction 
oceurs, in which one quantity of vapour arises, then we may write 
for (30): 


py, RT 
Sa glean Silig ela wile tae ele (31) 


Now AJ, is always positive in the binary system / + ZL -+ G, 
except between the minimum-melting point 7 and the point of 
maximumtemperature 7'7, where AJ, is negative. In fig. 4 AV, 
is consequently negative for liquids between /’ and H, positive for 
all other liquids on the side BC. 

—y is positive, when the liquid is situated between # and C, 
negative when the liquid is situated between / and B (figs. 2—4). 

—y, is positive, when the vapour is situated between /’ and C, 
negative when the vapour is situated between /’ and B (figs 2—4). 

In the points A of figs. 2—4 is AV,>0, /’—y>0and /?—y,>0; 
from (31) follows therefore dP <0. From each of the points / 
the pressure must, therefore, decrease along the saturationcurves, we 
see that this is in accordance with the direction of the arrows in 
the vicinity of the points / (figs. 2 -4). 

In the point » of fig. 2 is AV, >0, 7—y <0 and (?—y, <0; 
from (81) follows, therefore dP <0. Consequently we find that 


180 


the pressure in fig. 2. must decrease from n along the saturations 
curve, which is in accordance with fig. 2. 

In the point 2 of figure 3 is AV, >0, P—y<Oand ?—y, >0; 
from (31) follows, therefore dP > 0. Consequently the pressure 
must increase from the point 2 in fig. 3 along the saturationcurve. 
which is in accordance with fig. 3. 

In the point 2 of curve 5 in fig. 4 is OV, <0, ;“—y > 0 and 
8— 7, >0; from (31) follows, therefore dP>0. Consequently 
the pressure must increase from n along curve 5, which is in 
accordance with the direction of the arrows. 

We may summarise the above-mentioned results also in the 
following way: when to the binary equilibrium + 2-+-G (in which 
F’ is a compound of two volatile components) at a constant tempera- 
inre we add a substance, which is not volatile, then the pressure 
increases when the binary equilibrium is between the point of 
maximum-sablimation 7Z'~ and the point of maximum temperature 
7; in all other cases the pressure decreases. 


In the consideration of the general case, that the vapour contains 
the three components (XI and XII) we have deduced that the 
saturationcurves under their own vapourpressure can disappear in 
two ways at increase of pressure. 

1. The saturationcurve of the temperature 7’7 disappears in the 
point #7 on the side BC |fig. 5 (XD)]. 

2. The saturationeurve of the temperature 77 touches the side BC 
in the point 7 and is further situated within the triangle ; at further 
increase of 7’ it forms a closed curve situated within the triangle, 
which disappears at 7’z in a point within the triangle | fig. 6 (XJ)]. 

In the case now under consideration, that the vapour consists only 
of B and C, only the case 1 oceurs; this has already been discussed 
above and is represented in fig. 4. It follows already immediately 
from the following that the case 2 cannot occur. On a closed 
saturationcurve under its Own vapourpressure a point of maximum- 
and a point of minimumpressure occurs. On the curves now under 
consideration only, as we saw before, a point of minimumpressure 
can occur, so that closed saturationcurves are impossible. 

We may deduce this also in the following way and we may 
prove at the same time these curves, just as in the general case, to 
be parabolas in the vicinity of 77. 

When we consider the binary equilibrium #’+ liquid AH + 
vapour, then «=O; we equate y=y,, y,=~y,., and the pressure 
= Py. To this equilibrium applies: 


Be NG) ee Ze We | 
(Of = (Y,—i?) = — G60 Z, - (fon ) - 50) 
Oy OY, (32) 
dU . OZ, 
dy e on, 
further we have: 
(Y:-0—/?) a =F (F—y,) V, =r [%o— Yao] v= 0 as (33) 
which condition we may also write: 
Wee U Va == V, = V 
= a (34) 


y—0 = Yr — [2 ee 
For a ternary equilibrium /’+ 4 + G, the liquid of which is 
situated in the vicinity of point //, the pressure is equal to 
Ba «, f= Ss, 7, 4 and 7, 7. 7,- 
The three equations (17) pass then, when we use the conditions 
(22) into: 


Ss RSI. Hy AYL=0 (85) 


RTE+[v-V] a+ 4r&? + 4tn?+-4 (5 
dv oOoV 


[p—V,] a ate $e, LF =e 2 Gan a) Sd <5 5 OG: 4 (y,—/?) L, =? (36) 


iS ee va ae th sap kes os ot * (S18) 
Herein is: 
2 OV Os Ot 0?V 
Ts EAR fey foo toe ES hE Wee yth 

Oy Ow ~ OY dyOP 

(38) 
4 Os 3 0?V 07V 
a! Sam oe 

TE. Ov, ne ot, 0°V, OPA as 6 
—=i fey a un —_— enc 3¢ 
fig Malka hag apt og eS (89) 


In (35) and o6 Y, and y)9 are replaced by y and y,; we shall 
do the same in the following equations. When we multiply (385) 
by y,— and (86) by y—@, then it follows with the aid of (37) that: 

(y,—B) RTS + 2 (y,—B) 7 & + § (y—B) ty’ —3 (y—B) t, 1," 


mitre dV ( 2) OV. Ov are UTES 
AF 2 (( UP) dP ts y ey) =e = i= ap +(y, —B)sSy—= ( ) 


From (36), (87), and (40) it follows that this can be satisfied by: 
7, Of the order -, 4 of the order a and § of the order 2°. 
From (35), (86) and (37) then follows: 


OV OV, 
i —— |o and t.y, =(|u— a. . . (41) 
Oy Oy, 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


182 


Substituting these values in (40) we find: 
2): (4. —=B) RLS ears. al A ose oe emer es) 
wherein a has the same value as in (21) (XII). 
From this it follows with the aid of the first relation (41) that: 


at 


2 (y,— 8) RT § = —_.__7?. ... . (43) 


In the same way as in (XII) we find that we may write for this: 

j2 
t® (y—B) (y,—y) — 
Sa (y—B) (1 —9) ao 
PRT == 


WW. és) 


d*l 
LP? 
curve going in fig. 4 through the point H is parabolically curved 
in this point and touches the side LC in this point. 


d?l 
As in this point y—-8<0, y,—y <0, y,—8< 0 and TP >; 
a 


§ is always negative. From this it follows that this parabola has 
only the point 47 in common with the triangle and is further 
situated completely outside the triangle. Consequently only the point 
H vepresents a liquid; its other points have no meaning. 


wherein is fixed by (24) (XID. From this it follows that the 


(To be continued). 


Chemistry. — “The system Ammonia-water’. By Prof. A. Smits 
and S$. Postma. (Communicated by Prof. J. D. vy. p. Waats). 


(Communicated in the meeting of May 30, 1914). 


After the preliminary communication’) on this subject the inves- 
tigation of the system NH,-H,O has been continued in different 
directions, and it has now been completed. 

The continued research was directed in the first place to the 
accurate determination of the meltingpoint lines, corresponding 
with the pressure of one atmosphere. These determinations, which 
were now carried out by means of a gauged resistance thermo- 


1) These Proc. XII, p. 186. 


183 
. 
meter’), as is in use in this laboratory *), gave the following result. 
} . <9 
) (Method of procedure : supercooling a little and then seeding). 
[initia eee 
Concentration point of par peut 
mixture solidifica- | ti 
tion cauon 
100 mol. 9%) NH; | — 77.6°. 
94.7 = 80.9" | 
90.4 — 83.7 | 
86.5 — 87.2 
— 92.4 
81.55 
— 92.6 | — 92.5° 
78.45 = 68 Tee 92.5: 
73.5 — 82.2 | — 92.6 
71.1 — 80.3 
69.9 = TOT | 
66.7 — 718.8 
65.8 —— 18.9) 
64.6 — 719.2 
62.0 — 81.0 
61.3 — 81.7 | — 86.0 
60.7 — 82.3 iors 86.0 
60.3 — 82.9 — 86.0 
59.0 = 85,2) |= 8548 
51.0 — 84.1 | — 8.8 
53.0 — 80.2 
50.2 — 79.1 
50.1 — 79.0 | 
49.3 == 719.0) | 
43.9 | — 83.0 | 
42.2 — 86.0 | 
1) Gauging points were: melting ice 0°, melting mercury — 38.85°. Boiling 
CO, + alcohol — 78.34° + 0.20 (B—76). Boiling point of oxygen — 182.8° 4- 0.56 
(B — 76). 
2) Cf. pe Leeuw. Z.f. phys. Chem. 77, 603 (1911). 
: 13* 


184 


jneulritia| al = eee 
Concen- : Final point 
tration Point. oF of solidifi- 
mixture on cation 
40.6 — 88.2) 
39.8 = O07 | 
39.1 == Ol7 
35.75 =5 Ohi 
34.5 — 100.3 
34.0 — 96.7 | 
32.6 == 789.24) 
29.7 1492 | 
28.7 = (F353:| 
27.6 | 163i 
26.55 | — 50.4 
| 
23.0 | — 43.5 
20.2 | = 3440 
17.9 | — 28.6 | 
| 
4.46 | — 4.8 
0:0) 9 0.0 
| 


This result is expressed in Fig. 1. 
From this 7-X fig. follows : 
for the point of solidification of the compound 2 NH,.H,O0—78°.9. 
ra) ie a 5g - NH,.H,O—79°.0 
Further the eutectic point of NH, + 2 NH,.H,O + IL appears to lie 
at 81.4°/, NH, and — 92.5°. 
a ss yf , of 2NH,.H,O-+-NH,.H,O-+ L appears to 
lie at 58.5 °/, NH, and — 86.0°. 
3 . or ,» of NH,.H,O + H,O +L appears to le 
at 34.7 NH, and — 100.3°. 
Great difficulties were experienced in the case of the mixtures 
with less than 50°/, NH,, in consequence of the great viscosity of 
these mixtures at low temperature. 
Shortly after our just mentioned preliminary communication a 
treatise on the same subject by Rupert’) appeared in Journ. Am, 
Chem. Soc. 81 866 (Aug. 1909). 


1) Buriher Goinammenien Journ. Am. Chem. Soc. 82. 748 (1910). 


30) 


~b0} 


~100+ 


ee oe — re = = 
Ny 10 50 YW kD 60 Wiha 40 30 20 10 0 
X 


Fig. 1. 


As point of solidification Ruprrt determines the point at which 
the crystals brought into the liquid no longer grow or disappear. 
He measures the temperature accurate down to 0°.5 with a verified 


toluol-thermometer. Below —- 100° he uses a thermo-element, tested 
by comparison with the toluol thermometer and with the boiling 


point of liquid air. He himself considers the determinations with 
this thermo-element insufficient, which tallies with our results, as by 
extrapolation about —125° may be derived from Rupurv’s investigation 
for the temperature of the eutectic point NH,.H,O + H,O + L, 
whereas this point lies certainly 24° higher according to Fig. 1. 

Leaving the region of concentration 80—40°/, out of account, the 
agreement between Ruprrt’s results and ours is fairly satisfactory. 
If we compare the principal points, we get what follows: 


186 


REET Oe 


| 


Observer NH; 2NH3.H_O | NH,.H:0 
RUPERT. = 16220 se eo nO sale 28 
2 | | | 
Smits, Postma | — 77.°6 | — 78.°8 79.°0 
| 
Observer Eutecticum | Concentration Temperature 
RUPERT. NH; -+ 2NH3.H20 + L 81.2 mol. 9/9 NH3 — 94.°0 
S. P. | F fe , VSIRS Leena — 92.50 
| 
RUPERT. 2NH3.H,0 + NH3.H,0+L /|57.9 _, il — 87.0 
| 
See 5 = Sholay ‘ — 85.9° 
NH; .H,O0 + H,0 + L not determined by RUPERT 
. ee . r 34.7mol.%)NH3|}  — 100.3° 


It is at onee apparent from the determination of the melting-point 
diagram that the two chemical compounds, one with 2 mol. of 
NH, to 1 mol. of H,O, and the other with 1 mol. of NH, to 1 mol. 
of H,O are already considerably dissociated in liquid state at the 
temperature of solidification. 


Boiling-point lines. 


After centainty had been obtained in the way described here 
about the existence of two solid compounds between NH, and H,O, 
it was of importance to examine whether the existence of these 
compounds in the liquid state would also follow from the boiling- 
pomt lines observed at different pressures. These determinations, 
which were carried out with an apparatus as was used by 
Dr. pe Leruw’), yielded the result that there was no indication to 
be perceived that could point to the existence of compounds in the 
liquid. Hence it followed from this that at the observed boiling 
temperature the dissociation was already too strong, and that the 
investigation has therefore to be continued at still lower pressures. 

As the dynamic method is attended with all kinds of difficulties 
at low pressire, it was desirable to apply the statistic and not the 
dynamic method in the continuation of this investigation, and deter- 
mine the vapour pressure line of different mixtures of definite 
concentration, from which the boiling-point lines and the p-a-lines 


1) ZA. phys. Chem. 77, 284 (1911). 


ee 


187 


might then be derived. This investigation, in which also the mixtures 
which had previously been investigated dynamically were verified, 
yielded the followimg result. 

The following mixtures were examined. 


88,0 mol. °/, NH, 54,7 mol. °/, NH, 
Sng Se a Sib) eee oo 
Oe ek hi = 39:7" ae 
TA Cie ee A. 35.97) een 
695 ee, 39:7. ae 
cn ee O35. Gi as, ae 


62,7 ”? ” ” 


the results of which are expressed in fig. 2. 


These vapour pressure lines enable us to read the corresponding 
boiling temperature for a definite pressure (see table I), hence to 
indicate the boiling-pomt lines, and that with an accuracy down to 
tenths of degrees, and it is also possible to indicate the vapour 
tension of different mixtures for a definite temperature (see table II), 
hence to find the (pz)y-lines with an-accuracy of + 0,5 m.m. Hg. 

Fig. 3 contains the boiling-point curves, from which it appears 


100 


90 


80 x Sstatisch 


Geng dynanr sch 
70 
Le 
60 
50 
40 
30 


20 


10 


-30 


-40 


-00 


Ty AV Bri E:T 


T-X- or boiling-point lines for different pressures. 


mol. % NH3 | fp = 50mm. | p= 100 mm. DAMEN SET p=380 mm. | P/=760 mm. 
100 SE AIGEGN lk == 6122: || ==! 6liz4y pe 3.35 | ==, 4653) plik = =03a04 
88.0 Seioe ale = Goro. ler S0tise | eesti 249.6)” N= °30.4 
84.1 — 741 Geo ates en — 400g |=729)3 
77.8 = 7.0) | = 6215) ||. = 563 i aI | == 40.5). | = 26-8 
74.6 = 170.85 | = Gl! =054,0\5 | = derae ele ergant — 25.4 
69.5 =ycs.6- 88 — 587 | 52.4 | = 438 | 2eae.gt || @= ong 
66.3 — 66.4 — 56.4 = 50.20 | 4 — 34.0 = 199 
62.7 63.6) |= 536 |} = 47.25 || — 48.6 | 230.9): = Sit 
54.7 2G! earns ee © eens eas | poe 
51.5 Seo 42.1 SES | Ewa. al KG a 
39.7 mar SSeORn tee COLI Oye 19: G2m | 10-20 = Ike a 
35.9 — 32.7 | —21.3 | —140 | — 44 | + 44 = 
32.7 wey 8c g5|| =e 1G iG wel le me OF 250 =Peco.6510|| 15,914 a 
25.6 aS eo Or ese fl) eee ode el ce ipe7s a Ps 

TABLE IL 
p-X-lines for different temperatures. 
; Le 
t=—10° | t= — 65° | t= — 55° | t = — 45° | r= — 35° | t = — 30° | t= — 250 

mol. °/) NH3 | pincm.Hg. Pp 7) 7) P p p 

— 
100 8.25 11.75 22.6 | 40.95 | 69.95 pe eae 
88.0 7.2 10.2 19.6 | 35.5 60.6 71.4 aa 
84.1 6.7 9.6 18.5 | 33.4 57.3 73.6 = 
71.8 5.8 46«| «8.4 1652) |). 12955 BO}pieleG5r0y a 
TAG) 15:3 (4a 14.9 | 27.4 47.2 61.0 | 77.4 
69.5 | 4.58 6.5 12TH esos ee 40] 52.5 | 66.8 
66.3 5 Sra ye os5) pale Waite Ona 20.5 | 36.0 46.9 | 59.7 
eS fees (eel Asse page 922 17.25 | 30.55 39.9) | = 
Sg ee Disie lee 5h 10.6 19.4 25.1 | 33.55 
Bie S eel see ane oil 1cGs 4.2 | 8.3 he abs 20.7 27.15 
39.7 | = | 0.85 1.41 3.08 | 6.1 8.3 | 11.0 
35.9 | = | oe + 1.1 2.15 4,35 | 5.9 | 7.95 
Sie 8) Wee i OL Ie) Oi8 16 | 3.15 be ate | 6.45 
Dotemie ese othe ye = 0.9 1.65 2.3 | 3.1 


190 
that even that corresponding to a pressure of 50 m.m. He. does not 
reveal anything about the existence ef compounds in the liquid 


phase; there is nothing to be detected here of a constriction at the 
place of the compounds, as was found by Dr. ArEn’) in his investiga- 


110) 


gop CM Ha. 


= 


90 


30 


io 


Suse 


ith +. 


NH; qa 


Fig. 4. 


tion of the system sulphur-chlorine, and by Dr. pr Lrruw’) in the 
system aldehyde-alcohol. 

Still more interesting is the consideration of the liquid lines of 
the (px)7-sections, which are represented in fig. 4 for the tempera- 


c 


mes ——= PH = SS a Re — die. 55°, —65°, and — 70°. *) 
1) Z. f. phys. Chem. 54, 55, (1906). 
2) loe. cit. 


8) The vapour phases of the mixtures need not be investigated, as it appeared 
from a preliminary investigation that they practically consisted only of NH at 
the examined temperatures, as was indeed to be expected a priori. 


era 


eS? i & 


191 


We sce that at all the temperatures mentioned here these liquid 


lines exhibit the type of negative liquid lines’), as was met with 
by Konxstamm and van Daursen’) for the system ether-cnloroform, 
and by Grrtacn*) for water and glycerin, while as Baknuis RoozeBoom 
remarked, such a line may also be derived from the investigation 
carried out by ScHREmNEMAKERS*) for the system acetone-phenol. 

Nor do liquid lines of the (px)7-sections give the least indication 
of the existence of compounds in the liquid phase, and it is most 
remarkable that this even applies to the liquid lines corresponding 
to a temperature of — 70°, so only 9° above the temperature at 
which the compounds separate out of the liquid; an indubitable 
proof therefore that the compounds found undergo a dissociation in 
the liquid, much greater than would have been expected. 

To complete the investigation the most important lines of the P7- 
projection of the spacial figure were also determined, the result of 
which is expressed in fig. 5, in which the three-phase lines of the 


two compounds are very apparent. The difference in triple point 
pressure of the two compounds.amounts to +17 m.m. Hg. 


Finally also the. plaitpoint curve was partially. determined; as was 
to be expected this curve does not present any particularity either. 


Anorg. Chem. Laboratory of the University. 


Amsterdam, May, 1914. 


1) Baxuuts Roozesoom. Die Heter. Gleichzew. Il 40 (1904). 
*) Verslagen d. Kon. Akad. v. Wet. 1901, 156. 

3) Z. f. anal. Chem. 24, 106 (1885). 

4) Z. f. phys. Chem. 39, 500 (1902), 


192 


Mathematics. — “On Hermite’s and Apri’s polynomia.” By 
N. G. W. H. Beverr. (Communicated by Prof. W. Kaprryy). 


(Communicated in the meeting of May 30, 1914). 


Prof. Kaprryn has deduced the following expansion ‘) : 
(a—b6x)? 


1 spe =a Or H,( oe) 


ee > —_— ep 

Vy (1—6’) 0 2n on! (1) 
in which #, (2) represent the polynomia of Hermite. Let in this 
expansion «=O, then we find: 


48 


(2) 


2x2 
1 ie _ 2, 6H,(2)H,(0) 
VO—é6’) R erie anal 
Now it holds good for the polynomia of Hermite that: 
i ue 
Hon+1 (0) = 0 Hz, (0) = (— 1)" x > ae) 
On account of which the above relation passes into: 
6272 
os ix eo == \(= 1p , Hen() (4) 
V(1—6’) 0 22n. nl 
For the polynomia ¢, (7) of ABEL we know the expansion: 
x9 
1 i= oo 
aay = San ety / > 6 ope 
If we replace in (4) 6? by 6 we find: 
62:2 
eae 18 eS (—1)" Hor(2) 
Vy (1—d) 0 222. mJ 
1 
If we multiply the first member of this relation by t——— and 
vy (1—6@) 
(2n)! 


2] 

the second member by 
. Q2n  (p!y2 

04 a (n!) 


to the first member of (5). By equalizing the coefficient of 4” in the 
two second members, we find the following relation between the 
polynomia of ABeL and those of Hermite: 


6”, the first member becomes equal 


yp (a= > | 1)jr-k (24)! — Ho, 9%(z) - (6) 
Q2n pe (k@—hE _. 


If we multiply both members o7 (6) by 
Hyp, —i (3) e—™ dx 


y These Proceedings. Vol. XVI, p. 1198 (22 


193 


and integrate between —o and + o, then we find by application 
of the well-known integrals : 


+a 
[eo (a) Ey, (a)\e—* dz == 0 moe n 


+a 
de (2) e—? da = 2" .m!i Yn: 
—on 


ae Qn—2i)M(2i! 
| in () Hon si(e) db = (=I) en 


Ss) 


~] 
— 


Prof. Kaprayn deduces the following representation by means of 
an integral for HeRmirr’s polynomia ') : 


Cae eae wn 
e — 7 
let @) = e *u cos { vu — — )du. 
n Va 9 
J 
0 


If we substitute this expression in (6): 


; ~=— 2h)! 
P(x’ )= : fe ae (S128 — y2n—2k eos (wu—(n—k) x) du 
22a k—=0 (k!)?(n—hk)! 


or, if we work out the cosine 


ao u? 
ex? —— n (2k)! p : 
Gila") = — e 4 cosaudu + ~ ) urxn—k) , . (8) 
221V/ ar, k=0 (k/)?(n—h)! 
0 
Now is 
8 
(2h)! = fe-wyhay 
0 
consequently 


f+ 2) 
7 Db)! n 2(n—k) < 
Ss ess y2(n—k) — S ee : “ yy dy a 
> (k(n —h)! 0 (k/)?(n—b)! ves 

v » (9) 


7° NOGA cant OE A ok 

ne 1 y 2k — y2n ul fn yi \2 
= yen e—vdy = ae : —— e—Ydy 2S = == 
i 0 (kL)? (n—h)I \u mi o KILE u 


For AseL’s polynomia we have: 


: ens al n\ (y \2* 
a ue een, k u 


1) lie. p. 1194 (9). 


so that we can write for (9) 


, oa 
yen y" 
€Yapn | ——, | du 
ni, w 
0 


Substituted in (8) we get the double integral 


io 2) 2 i 3) 
u 4 


ex? as 
D(a?) = EL fe 42"+1 cos wud | e—ul ep, (—t?) dt 
0 0 
if we introduce y = wt. 

By substitution of «= 2y it passes into 

im i] a) . 

e—¥ yn) cos Danydy | ee Pri—t*)dt . . (10) 

0 0 


Now we make use of the relation *) also deduced by Prof. Kaprnyn 


Pilz?) = nl 70 


n 


i t yo Prt) 
Bat = ea (11) 
(SED a) es 


vu 0 


In (10) we substitute «= ¢ and then. multiply both members by 


1 
e—t dt 
140 


and integrate between O and o, then we get by making use of (11): 


ive} 


+e) a) D 
3 tn 4 : ‘ 2yVt 
r ef : for y2n-l dy {e—20 Gn(—wu*) du ae gv" dt. 
A (1+¢t)"11 niV x, ‘ : : 1+t 
0 


0 0 


0 
According to a well-known integral in the theory of the integral- 
logarithm, 1s *) 


oo RD 


“cos 2ypt _ ( # cos 2yHa : ; 
| — dt==2 | SS hi, (e2)—ey li (e—2Y) 
: l+e 


consequently 


2) Lo) 
Ae = us = dt= oi ey" y2n+ie—2u]7 (e21/) or Uli(e —2y)'dy 
i (1+) nlm, : : : : 
0 0 (12) 
5 fens) du.\- 
0 | 
By summation from 7 =O to n= we find: 


1) lc. XV, p. 1250 (14). 
2) See for instance “Theorie des Integrallogarithmus Dr. Nietsen page 24. 


195 


oO 


ng ~ 
4 BREA a icy tees : Sryelrve 
ears e—#" e—24lt, (e7Y) + e2yli(e—2Y) dy | e—2y"'du >’: : Gf i(-u’*) 
a QO 7! 


0 10) 


Now is’): 
s 


am 


Pm (a) = e*J (2 az) 
m! 


2) 

> 
—_— 
) 


in which J, represents the function of BesskL of order zero. From 
this it ensues consequently that : 


yO 


4 i 
— Va, yie—2li, (é 27) + yli(e »—2y) iy fe e—2yu J. y(2iuy) lu. 


i) 


As is known, 
oa) y2ny2n 


Jy (Quy) 


u=0 (n We 
so 
« ) yen Jie] roa) if 7 
—2uy J, (Qiuy) du = + +— {- 2uyy2ndu= = ——— J e—% 22n dz — 
ot ive ~ aaa y(n!) 292n-+1 
0 0 v 
ee eee 
ay y(n 3 22n1 * 
Introducing this we have 
en (eee & 2n)! 
1 = — —— | [e—2v i, (ev) 4+. e2y li (e—2)] dy . 5 
Vn no (n/)?220+1 
0 
or 
l oD 
af — | [e—2y li, (29) + ey li (e—2y)] dy . (03) 
2n Me 
as 271 1 
Meciine to an integral used before, is 
ao D 
7 . DQ, 
fleom (e27) + e2yli(e—29) | dy=— :f tcostdt cen til 108 taretg =" dt . 
« Yas 
) 0 
Formula (18) may also be written as follows: 
1 4 ij AR 2y F ; 
= — lim costarctg—dt . . (14 
a (2n 1 Vz y=00 “¢ ! 
E = rest 0 
n=0\ 2 J 2241 
. . . an . . 
By multiplying formula (11) by ar and by summation from 2 = 0 
ni 


fo n =oo we find: 


1) These Proceedings XV, p 1246 (9). 


196 


et ey t n * e—! oOo at 
if OD) = 4) = J, (2V ct 
| Ie Ga 070 “lre) = ieee: 0 gs (0) Nike eres (2V at) 


0 0 


meat +(«—1)t 
‘| aS nae fr nevend 


0 


or 


(15) 


In order to deduce some more relations from formula (11) we set 
to work as follows. In Dr. Nianp’s dissertation’) the following 


relation is deduced for ABen’s polynomia: 
n—1 
= 
Gn (v=) = — = gx(e)- 
k=0 


By summation of formula (11) from 2=0 to n—1: 


on n—1 tn ie n—l 
,—t > = = n (t) dt 
Jere at a lee eae 
0 
or 
alae 1! ae ay lt 
FE A eu 
foams re Ok 
0 0 
or 


s t . 
aya | Ge 1 (t) dt 
fe py” al te ee 


0 


We integrate the second member partially : 
- 
| (l+¢+1 


et et 
ei pet ces a Ore Fe) Tey 


0 0 


ety, (t) dt = 


(16) 


aya! oe = 
——— +f Ta Gn (t) dt 4 (to Gn (t) dt . 
0 0 


Formula (16) passes into: 


Ae pr 
n n \d 
See =f Oe ee bias 


0 


or by application of (11): 


1) Over een bijzondere soort van geheele functién. Utrecht. 1896 p, 19. 


197 


& 
t 


tn n a eH 
e—t___ dt= | e—'—____dt -++- | ——_—_q, (#) dt. 
fi (Ite 4 (ah Say ay 
0 0 0 

The first integral of the second member we convey to the first 
member, and we find: 


fe ae dt = we t) dt ae 
“(pay =farp el Se aa 
0 


0 
If we apply the same process to this, and again to the result, 
ete., we find at last after m-fold appliance: 


na oO 
[ : tim : { et 5 
e— ana —————(pal(t) dt ee 8) 
7 (1 +4) J +o" ie ( 
0 0 
We can render this formula still more general by summation 
from 2 —0O to n= o after division by (—1)" m/; we get: 
iv 2) a 
fo fr Guat 
e—2t r= (|= ((a\@iig 6 6 6 6 (ale) 
| (i441 pg m) 
0 0 


We apply the process explained above to this again and by 
summation again after division by (—1)" m/ ete. we finally find: 


on trp Pn (¢) 
—kt ey, | aoe / a eee ; : ; ) 
Je (1+¢°+1 a [i (t+ kyr at (20) 


in which % and m represent positive integers. 
Of course a formula analogous to (12) may be deduced from this 


o 

53 un 

a 
J Gay 
0 

\ (21) 
«2 ® 
4 ie 2 > 0 da] > * > Fi 2 

— ey yar Je—2ykli, (224!) + e2ykli(e 2k) dy fe- 24 Pn (—#*) dt. 

mY a _ ; 

0 0 


By summation, formula (18) is, however, found again. 

The formulae (4) and (5) may also be used in order to express 
the polynomia 2, in g’s. For this purpose we multiply the two 
members of (5) by 

1 fire tetas 1 10:5 
eee ii ec OT Las saat ap ae 

By equalizing the coefficient of G' in the second member of the 

I4 

Proceedings Royal Acad. Amsterdam. Vol. XVIL. 


198 


equation, thus obtained, to the coefficient of 7’ in the second member 
of (4) we find: 
. eal n 1 1.8.5...(2k-8) : 

Hp,,(#)=(-1)" 22"! } pp(z?)- Se a Ts ORT aan Pn—K x") } (22) 

By means of this expression an integral may be deduced. 

For if we multiply both members by 

e— “ip (x) da 

after replacing 2? by « and if we then integrate between O and o, 
we find, using the following well-known formulae ') : 


wo 


fe m (x) Pn (vz) da = 0 m == x 
0 
a 
foro (cdo! 
- 0 
° l 1.5.5.. .(2n—2m— 3) 
=a ») Ho a) da = (-—1)"4+! 22n , SS, —— 
| é Pn (a) Foy (Y v) da ( 1) al nt (n m)! Dn—m 
7 
or after some reduction: 
: ni 
e— Pn (@?) Hon (x) ede —(— 1)"+12"-+-m—1 _____ 13.5... (2n —2m—8) (28) 
ys (n—m)! 
0 


maon—l. 
In the same way we find 


D 
. 


fe —2* Qn (&") Ho, (@) veda == (—1). 228-1 nr, 2a) 


vu 
0 
and 
—_ 
| e— @n—i- (a?) Hon (a) cde = (—1)s" 229 eee) 
0 


If we write formula (22) in this form: 
1 £m) 
Ph Ve —2 kd 


Fo,, (x) — (—1)" 22n mI 


Y nv") 4 pn—1 (27) Pi (v7) 


we know that) 


fo 2) 


ox? ¥ 
Ci oh (Ge) == mae —40 KT (2e)//a)da. 
0 


!) Dr. Nistann’s Dissertation page 11. 
*) These Proceedings XV. p. 1247. 


199 


This we substitute: 


io 3) 


il! a 
Hp,(a) = (—1)”. 22" Indep, (w?)—3nlg,—1(@’)— — @t fe*F,2e/ee 
Dae 
0 
Ls n! Aha - 
iin 
We further introduce: 
& 3 
(=) Sit 2 dt 
0 
and 
ta! @r—(2’) = ava is i) (2aVa)da . na” 1 fetentae 
0 
We find then: 
FF LIE [o-“Neavejtafet 23 ” ok tk 
0 0 
or ea, some reduction 
(—1)—! — Han (a) + 1! gy (0°) = 
Ee >. (26) 


= eee (2a a) da fe tt Weta ma | dt 
2Y/ x : : 
0 0 


For «=0, the following identities arise from the formulae (6) 


U 
and (22): 


mi \> 
x, (24I(2n—2k) )! ni? n\k 
a) se ——— or — 22n — > ——— (27) 
a kP(n—h)!? (2n)/ ro ( 2n 
2k 
and 
9, n 9 F 5) 
(Caren Sealer aes aieel Claeee 
n! 2 p= k! ok 
or 
St Stee | ay 
nf? ve 2 ke=2 KI Qk 
(2n)! 


14* 


200 


Chemistry. — “The metastability of the metals in consequence of 
allotropy and its significance for Chemistry, Physics, and 
Technics”. Il. By Prof. Ernst Conen. 


The specific heat of the metals 1. 


1. In my first paper ') on this subject I called attention to the 
fact that the physical constants of the metals hitherto known, are 
to be considered as entirely fortuitous values which depend on the 
previous thermal history of the material used. 

In that paper I wrote with regard to the specific heat of the 
metals: Considering, for instance, the important part whieb the 
specific heats of the metals have played in chemistry and physics 
during the last few years, it is evident that a revision of these 
constants is wanted. 


2. Reviewing the earlier literature dealing with this constant, I 
found that it contains already a number of data which prove unequi- 
vocally that the specific heat of the metals does indeed depend on 
their previous thermal history. 


Le Verrmr published in the year 1892 a paper *) “sur la 
chaleur spécifique des métaux”, in which he describes his measure- 
ments with copper, zine, lead, aluminium, and silver. The calorimetric 
determinations were carried out between O° and 1000° by the method 
of mixtures. The temperature of the metal at the moment at which 
it was brought into the calorimeter was determined by means of 
a Ln CHareLigr pyrometer. 


3. Le Verrier stated that the mean specific heat remains as a 
rule constant till 200—3800°, after which it changes abruptly, as 
Pioncuon *) also found in the case of iron, nickel and cobalt. 

The variation of the total heat (i.e. the quantity of heat required 
to raise the temperature of 1 gr. of the substance from 0° to # C.) 
with the temperature is consequently to be represented by a curve 
with breaks and not by a continuous one. 

In the neighbourhood of these breaks the condition of the metals 
is not only a function of the temperature, but also of their previous 
thermal history. 


‘) These Proc. 16, 632 (1912). 

2) CG. R. 114, 907 (1892). 

3) CG. R. 102, 675, 1454 (1886); 108, 1122 (1886). In full: Ann. de Chim. 
et de Phys. (6) 11, 33 (1887). 


201 


As a consequence of the retardations in the structural change 
(changements d’état) of the metal, a different value of the total heat 
is found on cooling from that on heating. 

If a certain piece of metal is cooled or heated repeatedly, differ- 
ent values for the total heat are found. If we start from a lower 
temperature and return to it after having overpassed the break 
in the curve of total heat, a closed and not a single curve is obtained. 


4. This result is in complete harmony with the dilatometric and 
electromotive force measurements carried out by myself in collabor- 
ation with messrs. He_berMAN and MoksveLp, on copper, cadmium, 
zine and bismuth, measurements which led to the conelusion men- 
tioned above. 


5. Le Verripr’s paper contains some interesting data which we 
shall now consider in connection with our dilatometrie and eleetro- 
motive force measurements. 

The curve representing the variation of the total heat of copper 
as a function of the temperature, consists of four parts. At 850° an 
absorption of 2 Cal. occurs; at 550° an absorption of 2 Cal.; while 
at 750°, 3.5 Cal. are absorbed. 

Thus, while our dilatometric measurements proved that there exist 
more than two modifications of copper, the same fact was noted a 
long time before by Lu Verripr, using a different method. 

The measurements of Le Verrigr which are summarized in table I, 
have, however, been quite overlooked hitherto. 

It may be pointed out here that the transition temperatures which 
can be deduced from Le Verrier’s determinations will generally be 
too high. This is a consequence of the retardation of the molecular 
changes, which were also observed by him. Fresh experiments with 
the pure modifications of the different metals will throw light upon 
this point. 


6. From the determinations of Lu Verrier there follows also, that 
there exists a transition point for lead which has so far been unknown. 
Experiments in this direction are in progress in my laboratory. 


7. The same may be said with regard to silver. 
8. Aluminium shows, according to Ly Verripr, an absorption of 


10 Cal. at 535°. It may be pointed out that Dirrensercer (Phys. 
Techn. Reichsanstalt at Charlottenburg—Berlin) proved ten years 


Temperature. 


0—230° 
220—250 


250—300 


O—110° 
100—140 very variable 


110—390 


300—400 


0—300° 
300—530 


202 


DABBLE 


Mean spec. heat. 


Pb. 


0.038 
Almost nil. 
0.0465 


0.096 


Total heat. 


0.038 X t 
Almost constant. 
8.15 + 0.0465 (#250) 


0.096 « ¢ 


absorption of 0.8 Cal. in 
the neighbourhood of 110° 


11.36 + 0.105 (¢ -110) . 


0.105 
31.4 + 0.122 (¢t- 300) 
0.122 \ increases rapidly above 400° and 
ra amounts to 46 Cal. in the neigh- 
bourhood of 410° immediately 
before melting. 
Al. 
0.22 0.22¢ 
0.30 


Te crystallization of the silicium 

| occurs at + 500° and the break 

530—560 ? lies with Al which contains Si in 
the neighbourhood of this tempe- 


rature 


65 + 0.30 (t-300) 


Absorption of 10 Cal. in the 
neighbourhood of 535° 


139 ++ 0.46 (t-530) 


540—S00 0.46 170 Cal. at + 600°; increases 
rapidly and exceeds 200 before 
melting (620°). 
Ag. 
O—260° 0.0565 0.0565 ¢ 
260—660 0.075 14.7 + 0.075 (f—260) 
44.7 + 0.066 (t-660) 
: : 62 Cal. at + 930, imme- 
660 —900 0.066 diately below the melt- 
ing point. 
Cu. 
0—360° 0.104 0.104 ¢ 
320—380 0.104 Absorption of 2 Cal. at + 350° 
360—580 0.125 37.2 + 0.125 (#360) 
560—690 0.125 Absorption of 2 Cal. at + 580° 
580—780 0.09 37 + 0.09 (¢—580) 
740—800 0.09 Absorption of 3.5 Cal. at + 780° 
780 —1000 0.118 eM N a aed 


117 Cal. at + 1020°. 


208 


after Le Verrier that this metal is capable of existing in more than 
one allotropic modification and he found a transition temperature 
between 500 and 600°. I hope shortly to report on this point, in 
connexion also with a question which is important from a technical 
standpoint i.e. the disintegration of aluminium objects at room tem- 
perature, a disease which is the cause of a good many complaints in 
industrial circles as well as in daily life. 


9. That others had never observed the phenomena described by 
Ly Verrier may be explained by the fact that they had not heated their 
preparations repeatedly to high temperatures, as he did. We have 
also observed during our dilatometric researches that such a transition 
point can be overpassed several hundreds of degrees without any effect. 
If on the contrary the metal is repeatedly cooled and heated the 
transition is “set going”. As the means of overcoming these retard- 
ations are now known we are able to avoid them. A systematic 
research in this direction is now possible and I hope to report 
shortly on it. 


Utrecht, June 1914. van “t Horr- Laboratory. 


Physics. — “Jleasurements of isotherms of hydragen at 20° C. and 
15°.5 C.” By Prof. Pa. Konystamm and Dr. K. W. Watsrra. 
Van per Waats fund researches N°. 7. (Communicated by 


Prof. J. D. vaAN DER Waats). 
(Communicated in the meeting of April 24, 1914). 


§ 1. Choice of the substance and the temperature. 


With the apparatus described in N’. 5 and 6 of this series we 
have made measurements of hydrogen isotherms at 20° C. and 
15°.5 C. This choice was led by the following considerations. As 
we already set forth in the beginning of Communication N°. 5, one 
of the motives of our research was the desire to be able to make 
an accurate comparison with the results obtained by AmaGat. Our 
first intention was to determine anew AMAGAT’s air isotherms; then 
we were, however, checked by peculiar difficulties. Every time, 
namely, when a measuring tube was filled with air in the way 
described in the previous Communication, and was then left for 


204 


some hours at high pressure, (above 1500 atm.), it appeared to be 
unfit for accurate measurements after that time. When the apparatus 
was opened, the mercury appeared to be quite contaminated, the 
glass tube and the platinum contacts being also covered by a black 
substance. 

Though in view of AmaGat’s experiments it could hardly be 
supposed that this substance was mercury oxide, formed by the 
action of the oxygen on the mercury, experiments of various kinds 
made it impossible to assume another cause. The supposition that at 
high pressure amalgamation of the platinum took place, proved 
erroneous, for in the black substance no trace of another metal than 
mercury could be demonstrated. Also the humidity of the air proved 
to be entirely without influence. When it finally appeared that neither 
filling with hydrogen nor with nitrogen yielded any trace, we 
could not but conclude that we had really to do here with the 
same phenomenon that Kurnen and Rosson‘) and Kurrsom*) had 
observed when using closed air-manometers, namely that oxygen and 
mereury act on each other at pressures of about 100 atm. KiEsom, 
however, describes a slow action, which only after the lapse of 
months manifests itself clearly; whereas we could demonstrate the 
formation of mercury oxide with certainty already after a few hours 
on account of the so much higher pressures. 

How it is that neither in his determination of air-isotherms nor 
in that of oxygen AmaGaT was troubled by this action, we cannot 
explain. After we had once ascertained it, the use of oxygen and 
oxygen mixtures was of course excluded. We therefore resolved to 
begin with measurements of hydrogen, which is most easily obtained 
in very pure state. The choice of the temperature of our measure- 
ments was directed by the desire to obtain a direct comparison with 
AMAGAT’s Measurements on oue side, and a supplement to SCHALKWIJK’S 
very accurate measurements at low pressures on the other side. 


§ 2. Filling of the apparatus with pure hydrogen. 

Most of our determinations have been made with hydrogen from 
the factory ‘Electro” at Amsterdam, which sells cylinders of com- 
pressed electrolytically prepared hydrogen. For the further purifi- 
cation and the filling of the apparatus with purified gas the arran- 
gement was used of which fig. 12 gives a schematic representation. 
It fits on to the most lefthand part of fig. 6 at /. 


1) Phil. Mag. Jan. 1902, p. 150. 
*) Diss. p. 50—53. Thesis III. 


205 


A horizontal glass tibe «@ passes on the lefthand side into a 
vertical tube c via an emergency reservoir 4. The tube c ean be 
fastened to the Gaedepump by means of a glass spring and a ground 


joint piece. In the middle of the tube @ is a three-way-cock <A, 
which gives access to a vertical tube d. A tube e is fused on to 
d, the former being provided with a cathode and an anode, which 
are connected with the secondary wire of a Ruhmkorff bobbin. The 
primary wire is simply connected with the electric light bebind an 
incandescent lamp. The purpose of this tube will be mentioned 
presently. Attached to @ is a branch tube 7, bent downward, which 
may be considered as one of the limbs of a siphon barometer. The 
other leg yg of the barometer is fastened to the righthand part of 
the tube a. In this there is another three way-cock 6 with a branch 
tube 4. To suck the mereury easily into the barometer tubes, resp. 
to expel it from them, a vertical tube with cock C is adjusted into 
the transition from / to g. On the tubes / and g, which are filled 
halfway with mereury, millimeter divisions have been etched to a 
height of 1 m. To make the mercury mirrors visible at a great 
distance care has been taken that a lamp can be slid up and down 
behind these tubes, a strip of ground glass between the lamp and 
the tubes intercepting the heat and making the light more diffuse. 
To the right of the place where the tube g opens into a, the latter 
is bent downward, and passes into a wider tube 4, This tube is 


206 


provided with four branch tubes, which can all be shut off by cocks 
secured by mercury. For the filling with a single gas the presence 
of two of these branch tubes is sufficient, namely / and m, resp. 
with the cocks D and /. Tube / leads, as appears from the fig., 
to the mixing vessel, in which the normal volume at 1 atmosphere 
can be determined. The tube m leads to the gas reservoir via the 
purification apparatus. This gas reservoir is in casu a cylinder of 
hydrogen as said above. The rubber tube, which is connected with 
the pressure regulator, is fastened on the other side with solution to 
a horizontal glass tube 7. This tube 7 has a vertical side tube s, 
+ 1 m. long and ending at the bottom into a vessel with mercury. 
Further 7 is connected by means of a rubber tube to a tube of infusible 
class g, Which is filled with platinum asbestos. The latter tube is 
connected again by means of a rubber tube to an ordinary drying tube 
p, with phosphorpentoxide, and the latter tube is again in connection by 
means of rubber with the above mentioned tube m. All the closures 
of rubber to glass are secured with solution. > 

In order to fill the measuring tube with pure hydrogen, the cocks 
BE, D, and F’ are opened after the already mentioned operations 
(Comm. N°. 6, p. 828). The position of three-way-cock A is such 
that both sides of @ are in communication with d. The three-way- 
cock B shuts off the tube g at the top. Position I. 

The airjet or oil-pump is made to serve in the beginning, the 
Gaede-pump completing the evacuation. When the air is sufficiently 
rarefied, the cock /’ is closed, and the empty tubes m, p,q, and r 
are filled with hydrogen from the cylinder. The mercury, which in 
the tube s has risen to barometer height in the meantime, will 
deseend; the mereury difference in the tubes / and g still indicating 
the barometric height.’) Then the hardglass tube g is heated, till 
the platinum asbestos begins to glow. The cock # is slowly opened. 
And while the gas is flowing into the empty space & and further, 
the hydrogen tube is again opened, so that the pressure in the tubes 
in, pg, and + always remains + 1 atm. This is desirable because 
in case of too great rarefaction the glowing hardglass tube g indents, 
and soon gives way. The gas that flows through mm to the different 
tubes, is almost pure, for the oxygen, for so far as it is present in 
ihe electrolytic-factory hydrogen, is quite combined with hydrogen 
to water throngh the catalytic action of glowing platinum asbestos, 

1) On account of an eventually too high pressure the tubes m, p, q, and r 
might burst now, if the open tube s with mercury safety valve had not been 


added. 


207 


and the water formed is entirely retained in the phosphorus pentoxide 
tube p. When the mercury in f and g is again at the same level, 
it may be assumed that everything is filled with hydrogen of one 
atmosphere. Now the cock / is again closed; / and the other tubes 
are again evacuated. An idea about the purity of the gas which 
was found in the tubes after the first filling, is now given by the 
discharges in the cathode ray tube e. As long as traces of oxygen 


still contaminate the hydrogen (i.e. with air — and the presence 
of the latter appears at the same time — the only possible con- 


tamination) the tube will be filled with red light. When pure hydrogen 
has filled the tubes, the light will exhibit the well-known rice-colour. 
An opinion may then be formed at the same time about the degree 
of rarefaction attained, and also about the closure of different cocks 
and couplings. 

The tubes are then again filled with purified hydrogen, and after 
another evacuation and filling the purity of the gas in all the tubes 
may be safely assumed to be sufficient. Then the cock VD is closed, 
the mereury bulb (see Comm. N°. 6 p. 828) is raised, and the pure 
hydrogen is in the first “pressure stage” \see p. 823). Now for a control 
the cock # was always closed once more, and the part of the tubes 
k, a, gy, d, f, and e was exhausted, to ascertain the purity of the 
gas with which we are going to work by means of the colour of 
the discharge light. 

If, what need not yet be done, (p. 830) it is desired first to 
determine the normal volume of the gas at + 1 atm., before it is 
brought into the first “pressure stage’, /’ must be closed before the 
last filling. The difference in height between the mercury levels in 
Z and ¢, and also the temperature of the thermostat must be deter- 
mined. The barometric height can be read with the siphon baro- 
meter /, g.*) But now the tube / must be in communication with 
the outer air. This may be effected by turning the cocks uf and B 
90° in positive resp. negative direction (Position ID). Then the tube / 
gets into communication with the outer air via / and /. This remains 
the case with g. But to prevent the tubes d and 7 to get commu- 
nication with the outer air also the cock A must be turned, but in 
opposite direction. The determination of the normal volume in JV’ has, 
however, as said before, only sense when we wish to convey a 
quantity of gas quantitatively to the measuring tube, which has not 
yet been done. 

To ascertain whether sufficiently pure hydrogen was obtained in 


1) By means of a cathetometer and the scalar divisions etched on the tubes. 


208 


this way, we made also a series of experiments with distilled hydrogen 
from the Leyden laboratory. The quantity of admixtures had been 


estimated at at the most by Prof. Kamuriinga Onnes. We 


5000 
oladly avail ourselves of this opportunity to express our indebtedness 
to Prof. Kamertincu Onnes for his kindness. In the filling with this 
gas the purification apparatus could safely be omitted ; the cylinder 
was therefore immediately connected with the tube m. The results 
of the measurements with this agreed within the limits of the errors 
of observation with the results obtained with the gas purified by 
us in the way described above. 


§ 3. The measurements. 


How through the different “pressure stages” the gas is conveyed 
io the measuring tube, has already been described above. Also how 
the temperature is then kept constant. This is seen by the deviation 
of the galvanometer, inserted into the Wuratstonr bridge. To get 
a first idea the pressure at which the galvanometer needle deviates 
is read on the manometer, and a corresponding number of weights 
is placed on the rotating pressure gauge, after it has been brought 
in communication with the tubes. If the number of rotating weights 
is too great, some are taken off till the galvanometer needle has 
returned to its original zero position. At last a final condition is 
reached, in which the putting on of 50 grams on the rotating weights 
makes the needle deviate, while the needle returns to its position 
of equilibrium when this weight is removed. 

The accuracy with which the pressures are thus measured on the 
small and the large pressure balance generally amounts to this 25 
erams up to 900 atmospheres. When the measurement is made with 
the small pressure balance, which goes up to 250 kg. per em*. the 
galvanometer needle may be made to deviate and return by putting 
on or taking away 10 grams, and even when the contacts are very 
clean with less. As, however, 25 gr. implies already an accuracy 
of 1 to 10.000, whieh is not reached on account of other sources 
of error, there is no sense in going so far in the determination of 
the pressure. We only mention the fact as a proof of the very great 
accuracy of the pressure balance for relative pressure measurements. 

When one pressure measurement has thus been made, the pressure 
is increased. The galvanometer needle, which now would continue 
to deviate, must again be brought back to zero, because now another 
resistance of the volume wire is measured, 


209 

Thus for every platinum contact in the measuring tube the pressure 
at the corresponding volume is determined. Then the pressure is 
diminished, so that two series of observations of the same results 
must be obtained, but one passed through at increasing, the other 
at decreasing pressure. The pressure differences at two corresponding 
observations of two such series rarely amounted to more than 50 
grams. It must of course be continualiy verified whether the tem- 
perature differences inside and outside the measuring tube have 
disappeared. This has taken place when the resistance of the tem- 
perature wire (ef. Comm. 6 p. 833) has become constant. 

In the measurement of the highest pressures, so when the large 
“head” of the pressure balance is used, i.e. between 1200—2400 
atinospheres, the accuracy of the pressure measurement becomes less, 
especially on aceount of the increasing viscosity of the mineral oil 
used as transmission liquid. Yet the error will certainly remain 
below '/J00- 


§ 4. Determinations between 2 and 200 atms. 

As was already mentioned in Comm. 6 (p. 830) unforeseen diffi- 
culties prevented us from determining the normal volume of the 
quantity used in the apparatus itself. For the determination of the 
isotherm of 20° C. we could make use for the calculation of the 
normal volume of ScHALKWIJK’s measurements, as will become clear 
from the discussion of our results. Such data were wanting for 15°.5 ©, 
And in order to be able to carry out al! the same an accurate 
comparison with AMAGAT’s measurements, we have executed measure- 
ments at lower pressures at that very temperature. In this way a 
control was obtained whether the equation for low pressures derived 
from the measurements may be extrapolated. 

We shall return to these points when our results are discussed, 
and first give a description here of these measurements too. As we 
again wished to use a large quantity of gas, the iron vessel D used 
in the large apparatus was used as a pressure cylinder. We then 
could fill the piezometer with a quantity of gas of the order of 
magnitude of 1 liter at 1 atmosphere. 

The piezometer originally consists of two pieces. The upper part 
was as the upper reservoir of our ordinary measuring tubes. At the top 
at a (fig. 13) there are 4 etched lines to be used after the cleaning 
of the tube. Lower down there is a widening 4; under this a sealed 
in platinum wire c, and at last an etched scalar division d. This 
tube was connected with a capillary, and bent round. A_ platinum 
wire is sealed into the bent part. Here a current can enter, and 


210 


leave through the mereury at the wire sealed in higher. When we 
provide the side-tube with a scale, and fill everything with mereury, 
and place it in a waterbath, a very accurate gauging is again 
possible as described in Comm. 5 p. 766. We first gauge the dis- 
iances of the etehed lines, then the volume from these lines to the 
sealed in wire, and then from there to the etehed scalar division, 
and this division itself. 


a G 


Fig 13. Fig. 14. 


The large reservoir, which is to be sealed to this top piece is 
calibrated after this sealing, by tiling with mereury the volume 
from the scalar division on the top piece to the sealar division at 
the bottom on the bottom piece. 

We now know sufficiently accurately the volume from the etched 
lines to the sealed in wire, and from here to the sealar division 
under the large reservoir. The tube is now fused to at the upmost 


211 


line, and at the bottom a bent tube is added. The brass flanged tube 
i of the pressure cylinder had been previously cemented at ¢, and 
after a few drops of mereury have been brought into the large 
reservoir, the tube is evacuated and filled in a horizontal position. 
When the tube has been filled with pure hydrogen, it is put erect, 
and the drops of mercury shut off the gas from the outer air. Then 
the whole thing is placed in a waterbath of 15°.5, while the differ- 
ence in height of the mercury in the tubes / and g is read. As 
the volume up to the scalar divison, and the division itself too, has 
been gauged, we now know the volume of a definite quantity of 
hydrogen at about 1 atm. and the desired temperature. In order to 
determine the pressure accurately, the pressure of the outer air 
must of course also be determined, for which purpose the siphon 
barometer is again used (p. 205). 

We can further dispense with the side tube, for it only served 
to protect the mercury at the bottom of the tubes against the water. 
It is knocked off at g, and after the still remaining tube has been 
entirely filled with mercury, the whole arrangement is put in the 
pressure cylinder filled with mereury. The pressure cylinder is 
closed, and connected with the hydrostatic press, which connection 
is also in communication with the pressure balance. By means of a 
rubber stopper a glass cylinder provided with a side tube at the 
bottom and at the top is put round the projecting part, so that 
water of 15°.5 from a thermostat keeps the gas at the desired 
temperature. The current was closed on the iron pressure cylinder ; 
then it passed through the mercury, and. when the required height 
had been reached it passed further through the platinum wire. By 
means of the pressure balance the pressure at which the platinum 
wire is reached, hence the pressure at which the gas volume is 
diminished to the upper part, could be very accurately determined. 


§ 5. Corrections. 


Some corrections should be applied to the experimental results 
obtained in the above described way. First of all in the gauging 
the volume is obtained in gr. of mercury of a definite temperature. 
To reduce these values to the accurate volume in em‘. two reduct- 
ions must be applied. A reduction should take place to em*. by 
dividing the value in gr. of mereury by the specific gravity of 
mercury at the temperatures of the gauging. The specific gravity of 
mereury according to the Tables of Lanponr and Bérnsrein was 
used for this- reduction. Further the compressibility of the glass of 


212 


the measuring tube should be takea into account. The gauging takes 
place at J atm.; during the measurement the tube is subjected to 
a pressure on all sides, in consequence of which the volume decreases. 
As the correction in question is only a small one, we have thought 
that for our first calculations it would suffice if we took the com- 
pressibility of our glass equal to the valne determined by AmaGat. 
We have therefore put the factor of compressibility at 22 x 10-7 
and assumed this quantity to be constant between 1 and 2500 atms. 
Also to the values of the pressure read directly some corrections 
should be applied. The weights in kg. read on the pressure balance 
should first be reduced to ke. per em*. by taking the value of the 
effective area into account. In anticipation of the comparison of the 
small pressure balance with an open manometer of sufficient capa- 
city discussed in Comm. N°. 5 p. 759, we have assumed that the 
effective area of the small balance, the piston of which is as 
accurately as possible ground in at 1 em?*., really amounts to 1 em’. 
Since we wrote our first communication we have been greatly 
strengthened in the conviction that we cannot make great errors in 
this way, by the result of Grora Kuein’s research '). According to 
his investigations*) the error in consequence of the neglect of the 
difference between piston and cylinder sections for ScHArFER and 
BUDENBERG’s balance amounts to at most O.1°/,,, and the deviation of 
the indicated and the directly measured value of the difference of 
the two piston sections is 0.4°/,, in the case examined by him. 
Now the large pressure balance could be compared with the small 
pressure balance by méasuring the same point of the isotherm in 
the neighbourhood of 250 atms. first with the one, and then with 
the other. So the measuring tube with the galvanometer in connection 
with it ete. serves simply as a manoscope, to judge when in the 
use of the two balances the pressure is exactly equal. It then appeared 
from some observations carried out in this way that when the section 
of the small balance is put at = 1 em*., the section of the small 
head of the large balance must also be put at 1 em*. within the 
limits of the errors of observation. As at these pressures the errors 
of observation are very small as we saw above, and will certainly 
remain below 0,2°/,,, this result is a new confirmation of the great 
accuracy of the Scuirrer and BupeNnserG pressure balances, and it 
gives therefore a new support to the validity of the made supposition. 
In the same way a comparison was made between the small and 


1) Untersuchung und Kritik von Hochdruckmessern. Berlin 1909. 
2) sO! (Clty peel 


213 


the large head of the large pressure balance in the neighbourhood 
of 1200 atms. Instead of the theoretical numerical ratio +4, three 
measurements gave resp. the values 4,012, 4,015, 4,016, average 
4,014. The weights when the large head is used, must therefore be 
multiplied by this value. 

The thus obtained value for the pressure in the head must now 
still be corrected for the excess of pressure of one atmosphere, and 
for the hydrostatic pressure difference between the head of the 
pressure balance and the measuring tube on account of the mercury 
and oi! columns. ‘These liquid columns were roughly measured, in 
which 1 em. of mercury more or less need not be considered ; nor 
need the oscillations of the barometer be taken into account. 

Finally the thus obtained pressure had to be reduced to atmospheres 
of 1,0336 kg. per cm*. 

In table T. 


The column under v, indicates the weighed volume in er. of mercury. 
g g 4; 


- 3 » Pkg the number of kg. on the pressure balance. 

Dy oe - pe the pressure, corrected for hydrostatic pressure 
difference in kg. per em’. 

33 5 », p the corrected pressure in atmospheres. 

rn % »  § the ratio of the volume at 1 atm. and at the 


measured pressure in consequence of the com- 
pressibility of the glass. 
Bv, the product of 8 and »,. 


” > ” 
E *. , » the corrected volume in em*. 
5) 3 » pv the product of p and v. 
TWIN NSS MG TE, IU 
5), November 1912. 
E— 2025 
CE ——  —————— 
vg Pre Po p | > pug v Pr 


67.1491 195.850 194,750 188.419 | 0.99959 | 67.1216 | 4.95473 | 933.57 
55.0632 | 245.400 | 244.300 | 236.358 0.99948 | 55.0346 | 4.06250 960.26 


45.4959 | 306.575 | 206.175 | 296.222 | 0.99935 | 45.4663 | 3.35620 994.18 
| 


37.3710 | 390.200 | 389.800 | 377.128 0.99917 37.3400 | 2.75633 | 1039.49 
31.0962 | 494.550 | 494.150 | 478.086 0.99895 | 31.0636 | 2.29302 1096.26 


27.4110 | 587.000 | 586.600 | 567.531 099875 | 27.3756 | 2.02087 1146.91 
22.7296 | 769.500 | 769.100 744.098 | 0.99836 | 22.6923 1.67508 1246.42 
19.3102 | 992.625 | 992.225 | 959.970 | 0.99789 19.2695 1.42242 1365.48 


Proceedings Royal Acad. Amsterdam, Vol. XVII. 


214 


TABLE I. (Continued). 
November 21, 1912. 
t—20% 
Ys Pre | Pe p B Be, v | pv 
| 
90.3267 130.200 129.100 124,903 0.99973 | 90.3019 | 6.66580 832.58 
87.5019 134.700 133.600 129.257 0.99972 87.4774 | 6.45734 834.66 
85.4277 138.250 137.150 132.692 0.99971 85.4029 | 6.30420 | 836.52 
43.7526 | 292.925 | 292.525 | 283.016 | 0.99938 43.7255 | 3.22769 | 913.49 
34.5011 391.600 391.200 | 378.483 | 0.99917 | 34.4725 | 2.54466 | 963.11 
25.0070 | 599.600 | 599.200 | 579.721 | 0.99872 | 24.9750 | 1.84358 | 1068.76 
December !!/;5, 1912. 
6209) 
60.4928 222.500 221.400 214.203 | 0.99953 | 60.4644 | 4.46331 956.05 
58.0°61 233.000 231.900 | 224.361 0.99951 58.0676 4.28639 961.70 
55.9451 243.350 242.250 234.375 0.99948 | 55.9160 | 4.12756 967.40 
53.7822 254.700 253.600 245.356 0.99946 | 53.7532 | 3.96791 973.55 
48.5533 286.400 | 286.000 276.703 | 0.99939 | 48.5237 | 3.58188 991.07 
45.9361 306.000 305.600 295.665 | 0.99935 45.9062 | 3.38867 | 1001.91 
42.9934 331.450 | 331.050 | 320.288 | 0.99929 | 42.9629 | 3.17140 1015.72 
39.4220 | 368.750 368.350 | 356.376 | 0.99922 | 39.3913 | 2.90775 | 1036.25 
35.8492 | 415.575 | 415.175 | 401.679 | 0.99912 | 35.8177 | 2.64396 | 1061.99 
22.0889 | 814.000 | 813.600 | 787.152 | 0.99827 22.0507 1.62772 1281.24 
February 10, 1913. 
120% 
65.7937 225.050 = 223.950 += 216.670 +=: 0.99952 —s«65.7621 = 4.85437 ~—- 1051.80 
34.9813 485.200 484.800 469040 0.99897 34.9453 2.57956 1209.92 
27.9749 660,000 659.600 638.158 0.99860 27.9357 | 2.06214 1315.97 
21.3124 995.000 | 994.600 952268 0.99788 21.3470 1.57578 | 1516.32 


20S 
Ug Pre Po. p p Ug 
65.7937 | 220.200 219.100 | 211.929 | 099953 | 65.7628 | 
34.9813 472.950 472.550 | 457.188 0.99899 | 34.9460 
27.9749 | 641.825 641.425 | 620.574 | 0.99863 27.9366 
21.3924 | 964.100 963.700 | 932.372 | 0.99795 | 21.3486 
14.4836 487.750 1960.3 1896 6 0.99583 14.4232 
February 13, 1913. 
C=20' 
65.7937 196.850 195.750 | 189.391 | 0.99958 | 65.7661 
34.9813 416.300 415.900 | 402.382 0.99911 34.9502 
27.9149 558.800 558.400 | 540.251 | 0.99881 | 27.9416 | 
14.4836 , 400.250 1609.1 | 1556.8 0.99658 | 14.4341 
April 22/54, 1913. 
G— 7202. 
36.1414 351.450 351.050 339.643 0.99925 —-10.7858 
32.4244 402.700 402.300 389.221 0.99914 13.7748 
21.1098 | 720.400 720.000 696.590 | 0.99847 17.2937 
17.3297 | 980.000 | 979,600 | 947.755 0.99792 21,0775 
13.8172 , 361.000 1451.5, 1404.3 0.99692 | 32.3965 
10.8401 | 587.750 | 2361.7 | 2284.9 0.99497 36.1143 
April 22/94, 1913, 
E— Nde.08 
36.1414 345.900 | 345.500 | 334.272 | 0.99926 | 10.7864 
32.4244 395.950 395.550 | 382.691 | 0.99916 | 12.0677 
21.1098 708.200 | 707.800 684.791 | 0.99849 | 13.7753 
17.3297 | 964.100 | 963.700 932.374 | 0.99795 | 17.2942 
13.8172 | 355.750 | 1430.4 1383.9 0.99695 | 21.0779 
121097 457.000 | 1836.9 1777.2 0.99609 | 32.3972 
10.8401 580,250 2255.8 0.99504 36.1150 


215 


TABLE I. (Continued). 


2331.6 
| 


February !\/;2, 1913. 


4.85443 | 
2.57962 | 
2.06220 | 


1.57589 
1.06468 


4.85467 
2.57993 
2.06257 
1.06548 


2.6559 
2.3914 
1.5559 
1.2765 
1.0168 
0.7962 


2.6659 
2.3914 
1.5559 
1.2766 
1.0168 
0.8904 


0.7962 


Pov 


1029.03 
1179.37 
1279.75 
1469.32 


2019.27 


919.42 
1038.14 
1114.30 
1658.74 


905.45 
930.79 
1083.89 
1209.81 
1427.89 


1819.24 


891.16 
915.20 
1065.47 
1190.26 
1407.15 
1582.42 


1796.07 


15* 


TABLE I. (Continued). 
June 4, 1913, 


= ee 
he sae | 
Vg. Pre Po Pp p | pug | vb Pu 
a ee EEE eee eee ee 

64.3346 | 141.800 140.700 156.13 | 0.99970 | 64.315 4.7476 646.28 

| | | | 
59.8154 153.475 152.375 147.42 0.99968 | 59.796 | 4.4140 | 650.71 
27.1963 | 370.500 370.100 358.07 0.99921 | 27.714 2.0502 | 734.12 


21.2326 | 524.750 | 524.350 507.30 | 0.99888 21.209 1.5656 | 794.23 


16.2658 766.100 | 765.700 740.81 0.99837 16.239 1.1987 | 888.01 
| 
| | | 
12.1023 | 1236.000 | 1235.600 | 1195.4 0.99737 12.070 0.89097 | 1065.07 
| 


In conclusion we give the two observations at 15°.5 for the deter- 
mination of the compressibility between 100 atmospheres and atmos- 
pheric pressure. The first column gives the pressure in atm., the 
second the volume in em*. the third the product pe. 


ABE we 
November 1913. 
[5 == Va\ea), 
1.0384 | 484.6 503.19 
97.91 5.4474 | 533.35 


December 1913. 


as NSD 
| 
1.0004 | 536.07 | 536:28 


104.82 | 5.4474 570.99 


Amsterdam. Physical Lab. of the University. 


PACE 


Physics. — ‘The hydrogen isotherms of 20° C. and of 15°.5 C. between 
1 and 2200 atms.” By Dr. K. W. Watstra. Van per Waats’ 
fund researches N°. 8. (Communicated by Prof. J. D. van 
pER WAALS). 

(Communicated in the meeting of May 30, 1914). 
Tete er 

§ 1. Agreement of the observations below 1000 atms. with 
SCHALKWUK’S csotherms. 

For each of the series of observations given in the preceding 
Communication we have determined an empiric equation of the form ; 
PV=a+6D+cD+d. 

As only series of observations below 1000 atms. can be represented 
by this equation with 4 virial coefficients, only these series come 
into consideration for the present. The obtained observation material 
above 1000 atms. will have to be considerably extended to enable 
us to calculate the following virial coefficients with the same 
certainty. 

If of the above equation we wish to determine a, }, c, and d, 
we get a number of equations equal to the number of obser- 
vations, and consequently then with 4 unknown quantities. To 
solve these equations according to the method of least squares 
is not feasible, as then the normal equations become practically identical, 
which may already be seen beforehand. We have been able to apply 
Prof. E. v. pb. SANDE Bakunuizen’s method successfully, which was also 


ie— 202: 5), November 1912. T=20°. 21 November 1912. 
P | PH(O) | PYO) (AC) P| PY(O)| PY (0) | (O¥(C) 
| | 
959.97 1365.48 1365.48 0.00 579.72 1068.76 1068.76 0.00 
744.10 | 1246.42 1246.43 | —0.01 378.48 963.11 963.11, 0.00 
567.53 | 1146.91 1146.81 | +0.10 283.02 913.49 913.49 0.00 
478.09 | 1096.26 | 1096.42 —0.16 132.69 | 836.52) 936.49| 0.03 
371.13 1039.49 | 1039.49 0.00 129.26 | 834.66 834.66/ 0.00 
296.22 | 994 18, 993.95| + 0.23 124.90 | 832.58 | 832.55] +0.03 
236.36 | 960.26] 960.42] —0.16 PV =710.50 4311.45 D + 
188.42 | 933.57] 933.56) +0.01 Bie OE inte 02D 


PV = 829.71 + 445.08 D + 
+ 353.40 D2 + 197.28 D4. 


T=20?: N/;5 December 1912. Ti — 202% 10 February 1913. 
P| PV(O)| PY) | (O)(C) Pp | PY (OV PEG) Ae 
| | 

787.15 | 1281.24 | 1281.25) —0.01 962.27 | 1516.32 | 1516.32 0.00 
401.68 | 1061.99; 1062.00 —0.01 638.16 | 1315.97 | 1315.97, 0.00 
256.38 | 1036.25 1036.21 0.04 469.04 1209.92 1209.92. 0.00 
320.29 1015.72) 1015.76 —0.04 216.67 1051 80 | 1051.80. 0.00 

295.67 | 1001.91 1001.81 +0.10 PV = 923.03 + 508.75 D + 


+ 552.10 D2 + 296.55 D4. 
276.70 | 991.07; 991.12; —0.05 


245.36 | 973.55) 973.51) +0.04 
234.38 | 967.40) 967.35) +0.05 
224.36 | 961.70) 961.75) —0.05 
214.20 956.05 956.11 —0.06 


PV = 842.61 + 409.64 D + 
+ 423.18 D2+ 191.36 D4. 


used at Leyden for the calculation of Amacat’s values at the time. 
(See Comm. 71). In how far we have succeeded in determining 
the empiric equations may appear from the following tables. We 
have placed there side by side P, ’V(O) — observed pressure and 
pressure <X volume —, and PV((C) — caleulated with the known 
volume from the empiric equation ; (V0) —(C) the difference between 
the product PV following from the observaticn and that following 
from the formula. 


i202: 11,5 February 1913. i200: 22/5, April 1913. 
Jee IEMA (OD) | 1ZAUA(G)) | (0)-(C) Ie PV (0) | PV(C) | (O)-(C) 

932.37 | 1469.32 | 1469.32} 0.00 947.76 1209.81} 1209.81; 0.00 

620.57 | 1279.75 | 1279.75) 0.00 698.53 | 1086.84 1086.84 0.00 
| 

457.19 | 1179.37 | Bee 0.00 389.22 | 930.78 ae 0.00 

211.93 1029.03) 1209.03) 0.00 339.64 905.45) 905.45 0.00 
| | | | 

PY = 904.53 + 499.85 D + PV = 732.67 + 358.69 D+ 


++ 494.67 D2 + 298.61 D4. + 257.51 D2+- 101.20 D4. 


219 


4 


T =-20°. + June 1913. 


P PV (0) | PV(C) | (0)-(C) 

—— 

740.81 | 888.01 888.01 | + 0.00 
507.30 | 794.23 | 794.22 | + 0.01 
358.07 | 734.12 | 734.12 | + 0.00 
147.42 | 650.71 | 650.68 | + 0.03 
136.13 | 646.28 | 646.30 | — 0.02 


PV = 596.07 + 207.24 D+ 
+ 147.31 D2-+ 34.13 D4. 


To find out whether these series of observations are in harmony 
with each other, they can be brought in correspondence directly. 
We did so before, and found only a slight deviation between them. 
Besides it is also possible to try and make all the series of obser- 
vations agree with ScHALKWIUk’s isotherm, and then compare them 
also inter se. But then there must first be a reason to suppose that 
it was possible to make these observations agree with SCHALKWIJK’s, 
and this had soon appeared. When in December 1912 only three 
series of observations had been found, we caleulated from that 
which contained the greatest number of observations (Dec. ''/,, 1912) 
an empiric equation from four of the observations, viz. at 787.15, 
401,68, 320,29, 276,70 atms. 

The other observations of this series appeared to be in good 
agreement with the found equation : 

PV = 841.70 + 415.09 D + 414.10 D®? + 198.16 D*. 

Also the two series of observations of Nov. 1912 appeared to be 
in harmony with this. Then a comparison with ScHaLKwisk’s obser- 
vations was attempted by reduction of the above equation to one 
with the same virial coefficient: @ as SCHALKWIJK, viz. @ = 1.07258. 
This reduced equation then becomes: 

PV = 1.07258 + 0.0,6740 D + 0.0,8569 D? + 0.0,,6659 D*, 
SCHALKWIJK giving: 

PV = 1.07258 + 0.0,6671 D + 0.0,993 D?. 

This equation holds from 8 to 60 atms., ours from 200 to S00 
atms., but we are now going to try to extrapolate with respect to 
the region of the lower pressures in order to compare these extra- 
polations with SCHALKWIJK’s. 

The differences are most apparent when the product PV’ is deter- 


220 


mined from the two equations for different values for D, and the 
products are joined in the following tables. PJ (GS) is then calculated 


from ScHALKWIK’s equation with 3 virial coefficients; PV (P) from 

our provisional equation, 
D PY (S) | PVP) | (PS) D | PV(S)| PV(P) | (PS) 
| | 1.0733 | 1.0733 | 0.0000 100 | 1.1492 | 1.1486 | —0.0006 
10 | 1.0794 | 1.0794 | 0.0000 200 | 1.2457 | 1. 2427) —0.0030 
20 | 1.0863 | 1.0864 | +0.0001 300 |. 1.3621 | 1.3573 | — 0.0048 
30 | 1.0935 | 1.0936 | +0.0001 400 | 1.4983 | 1.4963 | —0.0020 
40 1.1009 | 1.1009 0.0000 500 | 1.6544 | 1.6654 | +0.0110 
50 | 1.1085 | 1.1084 | —0.0001 600 | 1.8303 | 1.8718 | 40.0415 
60 | 1.1162 | 1.1161 | —0.0001 700 | 2.0261 | 2.1241 | +0.0980 
70 | 1.1242 | 1.1240 | —0.0002 800 | 2.2418 | 2.4330 | +0.1912 
80 1.1324 | 1.1320 | —0.0004 900 | 2.4773 | 2.8102 | +0.3329 


90 1.1406 | 1.1402 | —0.0004 


The deviations found in this way from what follows from SCHALKWIJK’s 
equation with the extrapolations from our provisional equation 
appeared to be surprisingly small. Only at a density 100 or P= + 115 
atmosphere pressure the difference is greater than 1 per 2000, but this 
is far outside the region of ScHaLKWisk’s observations. At D = 200 
or P= + 250 atms. the difference becomes 1 per 400. Later on it 
diminishes again, and takes opposite sign, but D = 500 or P= + 890 
atms. lies again outside the region of our series of observations. 

In connection with the mutual correspondence of the series of 
observations, the possibility of an agreement with ScHALKwiJK has 
appeared from this. 

In order to be able to compare the 7 series of observations inter 
se, and judge at the same time about the agreement with ScHALKWIJK, 
we have reduced the 7 empiric equations in such a way that they 
give PV = 1.3573 for D=300. This is then in agreement with 
the above table. Then the equations become: 


1 PV =1.06625 + 0.0373496 D +.0.0375009 D2 + 0.0,,69144 D4. 5, Nov. 1912. 
Il PV =1.06917 +-0.0371540 D + 0.0;72697 D2 +. 0.0;299111 D4. 21 Nov. 1912. 
Ill PV = 1.07375 + 0.0,66523 D + 0.087561 D2 +0.0;,64295 D4, 1/49 Dec. 1912. 
IV PV = 1.06920 + 0.068353 D + 0.(1g85981 D2 + 0.0;262047 D4. 10 Febr. 1913. 
V PV = 1.06893 + 0.0362806 D + 0.081640 D2 + 0.0;:68826 D4. —'11/, Febr 1913. 


VI PV = 1.05753 + 0.0374726 D + 0.077437 D2 + 0.0}263400 D4. —22/g4 April 1913. 
Vil PV = 1.07341 +. 0.0;67205 D+ 0.086024 D2 +- 0.0,264632 D', 4 June 1913, 


221 


At 407.19 atms. (800 > 1.8573) the series of observations have 
now been reduced in agreement with each other. 

From these equations we calculate first the product PV for the 
densities 100, 200, 300, 400, and 500 for so far as the corresponding 
pressures lie in the region of observation of the series, and hence 
agreement may be expected. We then find : 


D100 | 200° | 300 | 400 +] 500 


I | 1.1491 | 1.2429 | 1.3573 | 1.4961 —_ 


I | 1.1491 | 1.2428 | 1.3573 1.4963 | ‘1.6654 
Il | = "1.2426 | 1.3573 “1.4959 | 1.6641 
Wil is | 1.2423 | 1.3573 - 1.4963 1.6650 
V | — | 1.2419 | 1.3573 | 1.4967 1.6653 
VI | = | oe | 1.3573 | 1.4966 | 1.6644 
Vit | a | 1.2430 | 1.3573 ae a 
~j—.. = eae ee 

Mean 1.1491.) 1.2427 | 1.3573 | 1.4963 1.6648 


Besides with the mutual agreement, we are struck here with the 
agreement of the mean values PV with those determined provisionally. 

We reproduce therefore this part of the table and place the mean 
values PV(M) by the side. 


D | PV(S) PVC) PV(M) 
| 
100 | 1.1492 1.1486 i.1491 


200 1.2457 (12427 | 1.2427 
300 | 1.3621 | 1.3573 | 1.3573 
400 1.4983 1.4963 1.4963 
500 1.6544 1.6654 1.6648 


It remained to draw up an equation which satisfies the last table 
of the mean values with a=1.07258 in accordance with SCHALKWIIk’s 
isotherm. This final equation drawn up for convenience with five 
virial coefficients, becomes: 

(). PV = 1.07258 + 0.0,6763D -+- 0.0,88215.D? 4 
+ 0.0,,66954.D* — 0.0, 151 D", 


5 


222 

This equation not only represents all our observations as well as 
possible; but the agreement with ScHALKWIJK’s results appears to be 
even better than for the provisional calculation, which is seen from 
the following table. 


| 
| 


D | PV(S)| PV(F)| (F)-(S) D | PV(S)| PV(F)| (F)-(S) 

1 1.0733 1.0733 0.0000 60 1.1162 | 1.1163 0.0001 
| | | | 

101.0794 1.0794 | 0.0000 70 | 1.1242 | 1.1242 | 0.0000 
| | | 

20. 1.0863 1.0864  +0.0001 80 1.1324 1.1324 0.0000 

30 1,0935 | 1.0936 40.0001 90 1.1406 1.1406 0.000 


40 1.1009 1.1010 | +0.0001 100 1.1492 1.1491 | — 0.0001 
50 | 1.1085 | 1.1086 | +0.0001 


The tinal equation may therefore be considered to represent the 
whole region of the isotherm below 1000 atms. The agreement with 
ScHaLkWik is perfect up to = 100, which corresponds with a 
pressure of 115 atms. Reversely it appears therefore that we may 
extrapolate up to +120 atms. from the equation at which ScHALKWIJK 
arrived from his observations from 8 to 60 atms., viz. 


PV =1.07258 + 0.0,6671 D + 0.06993 D?, 


At D= 200 or P=250 atms. the error which would 
then be made, becomes already 3 per 1000. For greater densities 
up to 2500 the number of virial coefficients 3 is too small. It 
must then be 4 at least. It will not do simply to add a 4" coeffi- 
cient to SCHALKWIJK’s equation, which appears from the deviations, 
which (see table) are now positive, now negative. 


§ 2. Comparison of the observations at J5°.5 with Amagat’s. 

We have one series of observations with 4 data below 1000 atms. 
and three above it at our disposal. (See p. 215). 

An equation has been calculated from the 4 data below 1000 as 
a control of the observations at + 100 atms. (See preceding com- 
munication). To compare our data with those of AmagaT at 15°.4 
we have calculated an empiric equation with 6 virial coefficients 
from 6 observations. In the seventh observation at 383 atms. we 
have then a control. 


P |PV (0)| PV(C)\ (OO 


2255.8 | 1796.07) 1796.07 0.00 
1777.2 | 1582.42) 1582.42; 0.00 
1383.9 | 1407.15 1407.15 0.00 
932.37 | 1190.26 | 1190.26 0.00 
684.79 1065.47 1065.47 0.00 
383.29 | 916.64) 916.66 —0.02 
334.27 891.16 891.16 0.60 
PV = 637.965 + 892.46 D = 735.72 D® + 1215.49 Dt — 
— 787.959 D® + 204.470 D*. 

With the value of PV at 700 atms. this equation is then reduced to: 
PV = 0.92967 + 0.0,18953 D — 0.0,22767 D? + 0.0,,79888 Dt — 
— 0.0,,10996 D® + 0.0,,60639 D*. 

The easiest way for the calculation is now to compare the pressures 

for the same volumes as Amacat. We then find: 


V | P(Am.) P(C) (C)-(Am ) 
0.002234 | 700 700 0 
0.002046 800 800.5 0.5 
0.001895 | 900 904.7 4.7 
0.001778 | 1000 | 1005.3 5.3 
0.001685 | 1100 | 1101.8 1.8 
0.001604 | 1200 | 1200.7 0.7 
0.001533 | 1300 1301.6 1.6 
0.001472 | 1400 | 1401.0 1.0 
0.001418 | 1500 | 1500.9 | 0.9 
0.001370 | 16c0 | 1601.1 | 1.1 
0.001326 | 1700 | 1704.2 4.2 
0.001288 | 1800 1804.2 4.2 
0.0012545 1900 | 1902.6 2.6 
0 0012225 2000 2008.0 8.0 
0.001194 | 2100 | 2113.6 | 13.6 
; | 


.0011685 | 2200 2220025) 20 ee 


These deviations and especially the progressive ones above 2000 
atms. cannot be explained from the temperature difference of 0°.1, 
among others on account of their irregularity. This would give a 
pressure difference of no more than 0.6 atm. at 2000 atms. For the 
rest the deviations are too large and too systematical to be con- 
sidered as accidental errors of observation. The most obvious explana- 
tion, a systematic error in the absolute pressure measurement made 
by Amagar or by us, cannot be accepted either, as it would yield 
a deviation proportional for large and for small pressures. Probably 
the same causes come into play, which also prevented agreement 
between AMaGaT and SCHALKWIJK’s observations. 


Amsterdam. Physical Laboratory of the Cuiversity 


Hydrostatics. — “The different ways of floating of an homogeneous 
cube.” By Prof. D. J. Korrewee. 


(Communicated in the meeting of May 30, 1914). 


This problem, whose treatment, however simple it may seem, 
offers considerable difficulties, was lately brought to a complete 
solution by Dr. P. Branpsen. 

If we limit ourselves to the cases in which the specific weight of 
the cube amounts to less than half of that of the liquid (which is 
allowed, because the other cases may be derived from it by inter- 
changing the floating and immersed parts) stable floating appears to 
be possible in four different possitions. 

In the jirst position four of the edges are vertical. It may be 
acquired for specific weights, expressed in that of the liquid, smaller 

1 1 : L 1 
than a Re Y 3= 0,211... For those smaller than e == (GG 
it is the only one possible. 

In the second position two of the faces are vertical, but the edges 
belonging to them are sloping. The surface section is consequently 
a rectangle. This manner of floating is possible between the specific 
weights 0,211 .... and O,25 

In the third position the space-diagonal of the cube is vertical 
and the surface section a hexagon. It is possible between the limits 
: and : of the specific weight. For the limits themselves the cube 
) a) 
is lifted or immersed just so far that the surface section, perpendi- 
cular to the space-diagonal, has passed into a triangle. Those limiting 
positions themselves are already unstable; consequently the stability 


225 


of this position disappears exactly there where for specific weights 
< — a hexagonal section becomes impossible on account of ARcHI- 
6 2 


MEDES’ Law. 

This third manner of floating was, probably for the first time, 
referred to in the ‘Mathematical Gazette” of Dee. 1908, Vol. 4, 
p. 338, Math. note N’. 285, in which note, however, the second 
one and the case now following was not referred to at all. 

In the fourth position one of the planes passing through two 
opposite parallel edges assumes the vertical direction. In this posi- 
tion one of these edges is partially immersed, the other one quite 
outside the liquid. In consequence of this the surface section is a 
pentagon for which the intersection of the liquid surface with the 
plane just mentioned is an axis of symmetry. 

Such ‘pentagonal’ floating can only exist, however, between 
narrow limits of density, viz. between the densities 0,226... and 
O,24... 

It should be observed that only the first and the second position 
gradually pass into each other; further that a completely unsymme- 
trical way of floating, in which neither one of the faces, nor one 
of the diagonal planes, nor a space-diagonal assumes the vertical 
position, cannot arise. 

One of the greatest difficulties connected with the problem consisted 
in the formal exclusion of such cases. 

It further appears that between definite limits of density, several 
positions, amounting at mosf to three, are possible for the same 
cube, viz., 

Below 0,166... the first position is the only possible. 

From 03166)... to. 0,211... the first and the third. 

From 0,211... to 0,226... the second and the third, 

From 0,226... to 0,24 ... (the limits of pentagonal floating) 

the second, the third and the fourth. 

From 0,24... to 0,25 the second and the third. 

Between 0,25 and 0,5 only the third. 

Strictly speaking one case in which one of the diagonal planes 
coincides with the liquid-level and the specific weight therefore 
anounts to exactly 0,5 ought to have been added to those mentioned 
above. Dr. Branpsen has indeed proved that stability exists in this 
case. Yet at the slightest alteration of the specific weight the adjacent 
positions of equilibrium become unstable, ei. those which arise by 


226 


lifting the eube a little or by immersing it in such a way that the 
diagonal plane mentioned remains parallel with the liquid-level. 


A paper by Dr. Branpsen in which the results described above 
are set forth and proved is going to appear in the “Nieuw Archief 
voor Wiskunde’ . 


Petrography. — “On some rocks of the Island of Taliabu (Sula 
Islands.) By Prof. Dr. A. WicHMANN. 


(Communicated in the meeting of May 30, 1914). 


After G. E. Rumpnivs had deseribed. towards the end of the 17th 
century, some jurassic fossils, originating from the east coast of 
Taliabu') it was not before the year 1899 that new geological inves- 
tigations were made again in the island mentioned above. It was 
R. D. M. Verseek who collected some rocks in some places of the 
north coast on the 4? and 5 of August and afterwards described 
them’). In November of the same year G. Bornm followed his 
example, and chose as point of departure of his investigations the 
findingplace mentioned by G. Rumpnivs, and afterwards continued 
his work over part of the south coast*). In December 1902, in 
January and especially during the months of October and November 
1904 an extensive part of the southern part of Taliabu was surveyed 
by J. W. van Novunuys*). The large collection gathered by him 
was described by G. Born‘), in so far as regards the fossils. In 
the following lines the communication of an investigation of the 
rocks may find a place. 


1) D’'Amboinsche Rariteitkamer. Amsterdam 1705, p.p. 253—255. 

2) Voorloopig Verslag over eene geologische reis door het Oostelijk gedeelte 
van den Indischen Archipel in 1899. Batavia 1900, p.p. 9, 10, 46, 47. — Molukken- 
Verslag. Jaarboek van het Mijnwezen van Ned. Indié. 37. 1908. Wetensch. ged. 
Batavia 1908, p.p. 20—21, 107108, 221223. 

3) Aus den Molukken. Zeitschr. d. D. geol. Ges. 54. 1902. p. 76. — Geologische 
Mitteilungen aus dem Indo-Australischen Archipel. N. Jahrb. f. Min. Beil. Bd. 27 
1906, p.p. 385—395. — Beitriige zur Geologie von Niederlindisch-Indien. Palaeon- 
toeraphica. Suppl. 1V. Stuttgart. 1904, p.p. 6, 13—14. 

) Maatschappij ter beverdering van het Natuurkundig Onderzoek der Neder- 
landsche Kolonién. Bulletin No. 48. 1905. — Bijdrage tot de kemnis van het eiland 
Taliaboe der Soela-groep (Moluksche Zee). Tijdschr K. Nederl. Aardrijksk. Genootsch. 
(2) 27. Leiden 1910, p.p. 945--976, 1173—1196. 

5) Beitriige zur Geologie von Niederliindisch-Indien. Palaeontographica. Suppl. LV 
1912, p.p. 123177. 


227 


Taliabu is a longitudinal island extending in the direction from 
East-West between 124°8’ and 124°41’ E. and 1°50’—2° S. Whilst 
the length amounts to 117 km., the width is no more than 387'/, 
km. A mountain range of an average height of 1000 to 1200 m. 
extends over its entire length. The formations of the northern part, 
hitherto little known, are restricted to old slate-rocks, quartzites, 
granite-porphyry and coral limestone, whiist on the southern part 
moreover extensive strata are found containing numerous fossils 
from the Jurassic system those of the Berriasien ineluded '). Among 
the eruptive rocks occurs especially much granite. Younger forma- 
tions play here likewise an inferior part, because the coral limestone 
is found only in the eastern half of the south-ecoast and no farther 
than cape Kona | Mantarara| ’). 

Granite. Van Novuvys already called the attention to the fact 
that the granites of Taliabu have much similarity with the granites 
deseribed by Verberk of the Banggai Islands, which are situated 
westward from the Sula Islands. They are characterized by the 
occurrence of dark red orthoclase, greenish dull white plagioclase, 
white quartz and black biotite*). Rocks in which the orthoclase is 
of a lighter colour are however not wanting in Taliabu. They are 
contrary to most granites of the Indian Archipelago, which as a 
rule are rich in plagioclase, to be regarded as normal biotite-granites, 
in which a more subordinate place is assigned to oligoclase. It 
appeared that mikrokline was always absent. The red colour of the ° 
orthoclase is caused by a finely distributed reddish brown substance, 
which disappears however as soon as the feldspar is altered into 
kaoline. Biotite is indeed always present, but sometimes very scarcely 
represented. It also occurs that by alteration it has been changed 
into chlorite, and then, at the same time, rutile-needles appear. 
Brown iron ore (limonite), in the shape of irregular flakes and aceu- 


1) J. Antpure asserts (Versuch einer geologischen Darstellung der Insel Celebes. 
Geolog. und paleontolog Abhandl. herausgeg. von J. F. Pompecxi und F. yon Huens. 
N. F. 12. Jena 1913, page 110), that among others also Lias is found in Taliabu. Most 
likely he mistakes — he is not so very particular — this island for Misol. Further, 
he says, with regard to the demarcation strata of the Jurassic and the Cretaceous 
system, that they “allerdings nach neueren Untersuchungen der Trias angehéren’’, 
There can neither be question of this, as is clearly proved by G. Borum’s essay 
(Palaeontographica. Suppl. IV. 1904, pp. 1—46). Most likely Antpure has in this 
respect mistaken Taliabu for Buru. (Vide: Centralblatt f. Mineralogie 1909, 
p. 561; 1910, p. 161). 

2) According to a communication of Mr. van Novnavys the coral limestone reaches 
only a height of + 10 m. 

8) Molukken-Verslag, p. 218, 


228 


mulations along the fissures is rather widely spread as a product 
of alteration. Apatite and titanite occur only sporadically. 

Van Novnvys has already aequainted us with the finding-places of 
the granites.') In the western part of the island we must mention 
the territory of Lekitobi in’ the first place. The hill westward from 
the entrance to the lagoon, the hills of the island Kona in the lagoon 
and likewise Tandjunge Merah the red cape — at the east side 
are all composed of this rock. The second granite-territory was 
found on the upper course of the Wai fa, where it borders upon 
strongly folded phyllite. 

The third region is situated northward from the Wai Taha and 
extends in the N.E. till beyond the left bank of the Wai Kabuta. 
A fourth area occurs on the upper course of the Wai Najo, where 
it borders the strata of the Jurassic system. South of this river rises 
moreover a granite-hill on the coast in the neighbourhood of cape 
Pasturi. The erratics that were found, besides in the rivers mentioned 
above, also in others namely Wai Miha, Wai Kilo, Wai Ila, Langsa, 
Wai Tabana and Wai Kasia point to the fact that granite is widely 
spread over the interior. H. Bickine finally mentions a biotite-granite 
containing hornblende from the Wai Husu °). : 

The contactmetamorphical formations, which have been caused 
by the eruption of the granites, deserve attention however in the 
first place, especially because both old slates and jurassic sediments 
have been concerned in it. 

On the northside of the lagoon Lekitobi an andalusite-mica-rock 
is found as a rock. In the pink compact rock macroscopically only 
numerous silver-white laminae of muscovite can be detected which, also 
according to the microscopic examination, form also the chief con- 
stituent. Besides the aggregates of these colourless laminae there are 
also those of irregular grains of quartz. 

The elongated prisms of andalusite are already to be recognized 
by their relief, they are nearly colourless in the thin sections and 
show no perceptible pleochroism. Rather numerous are the fluid- 
inclusions which they contain. As an accessory constituent tourmaline 
is present in the form of little strongly pleochroitical prisms (O = yellow 
to greenish-brown, E almost colourless). Ore is irregularly scattered in 
the form of black grains, and occurs moreover as a fine dust 

1) Bijdrage tot de kennis van het eilland Taliaboe, p. 949, 951, 963, 967, 971, 
972, 1174, 1178, 1180, 1184, 1185, 1190, 1191, 1193—1195. 

2) G. Bornm. Geologische Mittheilungen aus dem Ind. Australischen Archipel. 
Neues Jahrbuch fiir Min. Beil. Bd, 27. 1906 p. 93. 


229 


between the muscovite-laminae. As a product of alteration finally 
brown-iron-ore (limonite) is found. 

Andalusite-mica-schist. This hard, distinctly schistose, reddish-grey 
rock, in which the naked eye discerns only silvery muscovite-laminae, 
was found as a boulder only in the Wai Miha. In the thin sections 
the rock, of which quartz forms the principal constituent, shows a 
erystalloblastic structure. Numerous are likewise colourless laminae of 
muscovite, and besides those of a greenish mica. Andalusite is found 
in the form of colourless prisms stringed together and in grains, 
whilst prisms of tourmaline scarcely ever occur. Rutile forms dark- 
brownish red, very strongly refractory grains and knee-shaped twins. 

Mica-quartzite-schist. A boulder from the Wai Kabuta, a hard, 
grey and very fine-grained, distinctly stratified rock. Under the 
microscope we perceive that quartz, which is usually accompanied 
by muscovite, is the chief constituent, whilst in strata of a darker 
colour, but restricted to these, biotite is likewise freely spread. 
Moreover andalusite occurs in the form of aggregates of prisms, with 
numerous Ore-grains and further occasionally garnet, rutile, titanite 
and tourmaline. 

Mica-quartzite occurs among the boulders of the Betino, a left 
tributary river of the Wai Miha. In this fine-grained, reddish-grey 
rock numerous muscovite-laminae can be discerned by the naked 
eye. As appears from fig. I the quartz individuals do not exhibit, 
“Pflasterstructur’ under the microscope, but they engage into one 
another like teeth. Further it must be remarked that finely distributed 


16 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


230 


ironhydroxide has penetrated between the aggregates of muscovite. 
Though the rock does not contain andalusite, it is yet likely, that 
it belongs to the contactmetamorphie formations. 

Spotted clay slates such as Verbeek discovered ') in the isle of 
Labobo (Banggai Isles) were not found among the rocks of Taliabu. 

A group of rocks that have likewise been transformed by contact 
with granite, but belong to the Jurassic system, are of a quite different 
nature. Van Nounvys indicated already on his map a hornfelsmass 
in the region of the source of the Wai Najo, whilst for the rest he 
detected normal Jurassic sediments partly covered with alluvial 
sediments from the source of the river to its upper course. As 
appears from a subsequent investigation these hornfelshike masses 
belong to the calesilicate-rocks.*) Van Novnuys collected specimens 
of these in the Wai Najo and its right tributary, the Baja, and 
likewise in the Wai Tabana and the Langsa. They are all dense, 
very hard splintery and usually of a greenish-grey colour which, 
in some spots, changes into whitish and occasionally into dark 
crey. Some of those rocks as those of the Langsa consist of parallel 
strata sharply separated from one another, perceptible to the naked 
eye, and of a whitish- and blackish-grey colour. 

The epidote is a mineral, which, according to the microscopic 
examination, is never wanting, it is almost always represented by 
the optically-positive klinozoisite, which is usually colourless but 
oceasionally provided with a light-yellow tint. The always irregularly 
shaped grains can easily be recognized by their strongly refractory 
power and their other optical properties. Some parts of the /me- 
silicatehornfels originating from the Wai Najo consist chiefly of 
aggregates of this mineral, among which is found a_ colourless 
eroundmass that cannot be nearer defined and often contains infini- 
tesimal parts of dust. In other parts this groundmass forms the chief 
constituent of the rock, in which klinozoisite occurs then only in 
the form of isolated grains. 

Jesides the many and very little grains of klinozoisite in the 
lime-silicate hornfels found in the river Lanegsa, prisms of tourmaline 
and needles of rutile(?) were occasionally met with. According to 
the microscopic examination the difference between the light and 
the dark strata is only caused by the fact that the latter are rich 
in infinitesimal parts of dust. 


!) Molukken-Verslag, p. 219. 
2) Bijdrage tot de kennis van het eiland ‘Taliaboe, p. 1190, 1193, 1194, 
map N°, XX. 


9314 


The composition of a cale-silicate-hornfels from the Wai Najo is, 
according to the analysis of Prof. Dr. M. Dirrricn of Heidelberg, 


as follows: 


SOO Aa ee remem BAe ow Soe 58) 
DEG Os ee co ea le tu A tte BOCAS 
ATO ar Oe ee Se ee ee 
C0) Pee AP es ae ee Ge EOL 
C0 ere 1 A Ce 
iC Oma etn ee ee I Foe 6,02 
Mil Ore ear aey fo ees oh 5 POLS 
COD eee a ee OO) 
VIG ORE eee ae ne a ES By 
Oe pare ice eS ee, gee Tu Ses? OPT 
NG OMMe Penna cr wets ew ey, oh OR 
PAOD. Apts sh tei ie ee a 2 a hae Pe lee Me OR) Yo) 
COE Fee ee a ae) eee AOIGS 
PaO = (ind eredlOe\t et enw ee eames = (eI 7, 
1GPO (@ver TIO? to 1A). 4 5s iew 

100,40 


The specific weight is 3.213. From the analysis it appears that 
the result of the chemical composition in consequence of the contact- 
metamorphosis of the Jurassic marls is the disappearance of CO’, 
which, as in other similar rocks, is found only in a very slight 
quantity. The water was likewise for the greater part evacuated. 
A modification of the composition with regard to the other con- 
stituents cannot be observed. The results of the analyses of the cale- 
silicate rocks vary greatly, which is not astonishing on account of 
the great variety of the sediments that gave occasion to their 
formation. 

The fact that the youngest strata of the Jurassic system in Taliabu 
were interspersed with granite and metamorphosed, is of great im- 
portance; its eruption can consequently not have taken place earlier 
than during the Cretaceous system. 

The occurrence of granite of mesozoic age was hitherto only 
stated or made probable in the Malay peninsula by J. b, 
ScriveNor*), in Sumatra by Auc. Tosier’*) and R. D. M. Verser’), 


1) The Rocks of Pulau Ubin and Pulau Nanas (Singapore). Quart. Journ. Geolog. 
Soe. 66. London 1910. p. 429. — The Geologic History of the Malay Peninsula, 
Quart. Journ. Geolog. Soc. 69, London 1913, p. 351. 

2) Voorloopige mededeeling over de geologie van de residentie Djambi. Jaarboek 
van het Minwezen in Ned. Indié 39. 1910. Batavia 1912, p. 18S—19. 

3) Koloniaal-Aardrijkskundige Tentoonstelling. Amsterdam 1913. Catalogus, p. 76. 


16% 


232 


their statements were a short time ago confirmed by W. Vortz’). On 
the contrary J. Antpure writes: “Was das Verhalten der Gesteine 
“der Tinomboformation| zum Granit betrifft, so ist es immerhin von 
“Bedeutung, dass woh! nahezu alle echten Granite des Indischen 
“Archipels, vor allem die Granite von Malakka, Sumatra, 
“und Bangka, ebenso die grosse Granitplatte von Siidwestborneo, 
“paldozoischen und zwar in den meisten Fillen nachweislich*) kar- 
“bonischen Alters sind.” *) 

Mr. AnLBuRG is prudent enough not to mention the names of his 
informants. 

Graniie-porphyry. Hitherto this rock has only been found as erratic 
rock, namely by R. D. M. Versexk on the north coast, near Cape 
Damar *), by G. Borum in the Wai Kadai (described by H. BicKtne °) 
and by J. W. van Novusuys in the Wai Ha, a tributary of the Wai 
Miha. The granite-porphyry of the latter finding-place contains a 
yellowish brown, fine crystalline groundmass, in which numerous 
grains and dihexaedrons of quartz are inclosed. The light-yellowish 


crystals of ortheclase — sometimes twins according to the law of 
Karlsbad — are dull and have caused the formation of scaly mus- 


covite, as appears from the microscopic examination. They are 
moreover filled up with finely distributed brown iron ore. The much 
less numerous twinned individuals of plagioclase have caused 
similar alteration as the orthoclase. The crystals of quartz are 
characterized by numerous fluid-inclusions. Sometimes the intrusion 
of the groundmass is perceived, but glassy inclosures are utterly 
wanting. Dark constituents were only exceptionally found, and if so, 
in an entirely decomposed condition. The previous occurrence of 
biotite however is unmistakable, as the shapes of the laminae are 
found back in the limonite into which they have changed. The 
feldspars which form a part of the groundmass as well as the 
porphyrie crystals have caused a transformation into muscovite. 
Quartz-porphyry was collected by G. Borum in the Wai Husu 
and examined by H. bBickine. In Van -Nounvys’s collection are 
two specimens from the boulders of the Wai Najo. One is characterized 


1) Oberer Jura in West-Sumatra. Centralbl. f. Min. 1913, p. 757. — Stid-China 
und Nord-Sumatra. Mitteilungen des Ferd. y. Richthofen-Tages 1913. Berlin 1914, 
p. 37. 


2) The italics are mine. 

5) Versuch einer geologischen Darstellung der Insel Celebes. (Geolog. und 
palaeontologische Abh.dlg. von J. F. Pompeckr und Fr. Von Huens, N. F. 12. 
ane 1913, p. 28). 

) Molukken-Verslag, p. 223. 


5 G. Bornm. Neues aus dem Indo-Australischen Aretipel p. 391. 


233 


by a light brown groundmass, bearing great resemblance to the 
colour of chocolate, whilst that of the other specimen is yellowish 
brown. Microscopically the groundmass is like that of the porphyry 
from the Wai Husu microgranitic. The porphyrie erystals of quartz 
are bluish and attain a diameter of 2—4 mm. The flesh-coloured 
orthoclase crystals attain a length of about 1 em. Microscopically 
they are covered with a fine brown pigment and partly altered into 
an aggregate of little muscovite-scales. The groundmass is micro- 
granitic and consists of a fine aggregate of quartz and orthoclase. 

Syenite-porphyry. Only one specimen of this rock originating from 
the Wai Najo is present. With the naked eye only a few dark 
constituents can be detected in the grey to brownish dense ground-mass 
showing a somewhat violet tint, with the help of the magnifying glass 
likewise little rectangular sections of whitish grey feldspar can be 
discovered. From the microscopic examination it appears that they 
consist for the greater part of orthoclase, partly however also of 
plagioclase (oligoclase). The dark constituents are in the first place 
represented by green hornblende. The pleochroism is « = yellowish 
sreen, \=dark green, ¢—bluish green; ¢ >) Sa; ¢:¢ = 12°. 
Besides this biotite occurred frequently, which was however completely 
transformed into chlorite, whilst grains of ore and epidote were 
formed. Apatite is found in the shape of little thick prisms. The 
eroundmass is entirely crystalline and is composed of aggregates of 
particles of feldspar, among which a few little, angular grains of 
quartz occur. 

From the scarcity of porphyrie rocks in Taliabu may be deduced 
that originally they occurred only in the form of dikes. 

Diabase. ‘This kind of rock is likewise only represented by one 
specimen from the boulders of the Wai Kabuta. It is dull, greenish- 
grey and contains a few macroscopically observable dull-white 
erystals of feldspar. In thin sections the characteristic ophitic structure 
is to be observed, narrow and broader lath-shaped erystals of plagio- 
clase, between which the xenomorphic augites appear, which have 
undergone however partly an alteration into epidote. Grains of black 
ore are freely dispersed. On the fissures of the rock greenish-yellow 
epidotes have deposited themselves, which are accompanied by quartz. 


The oldest sediments found in Taliabu are represented — in so 
far as it is known — by phyllites, which have submitted to a very 


strong folding, as was already remarked by van Nounvys at the place 
mentioned. An extensive region is watered by the Wai Miha, i.e. 
from its source till it leaves the chasm between the Bapen Kudi and 
Bono Kedot6, whereupon it reappears again at Nali. In some spots 


234 


the rock contains strata and lenses of quartz and occasionally much 
pyrite‘). A second region that has not been thoroughly explored is 
found, according to the map, at the upper course of Wai Kabuta. 

Besides the finding-places mentioned above, van Nounuys mentions 
the river Langsa, but he remarks emphatically that the phyllites 
occur there only in boulders, but nowhere *) in the form of rocks. One 
of the specimens is composed of alternating thin, dark-coloured, 
almost black strata, and lighter brownish-grey strata more rich in 
quartz. From the microscopic examination it appears that biotite 
forms the chief constituent, occasionally accompanied by many grains 
of ore and fine black particles of dust and only few prisms of tour- 
maline and grains of titanite. The lighter strata consist chiefly of 
an ageregate of quartz grains among which are numerous little biotite- 
laminae. The rock is moreover penetrated in several directions by 
small veins of quartz, in which yellowish-green, wormshaped aggre- 
gates of little pleochroitical laminae of chlorite (helminth). 

Another phyllite is of a blackish-grey colour, dense and rather 
hard. In consequence of the decomposition of the rock such parts 
as are richer in quartz appear at the surface as knots. Microscopic- 
ally the little biotite-lamellae are irregularly spread over the quartz-mass, 
and sometimes closely compressed in accumulations. Sometimes a light 


1) Bijdrage tot de kennis van het eiland Taliabu, pp. 958, 961, 1174—1176, 
1187—1188. 
*) Page 1180. 


i) 


35 


sericitical mica occurs, and further prisms of tourmaline and ilmenite. 

The phyllites of the Wai Miha are usually softer than those of 
the Langsa, and the microscopic examination proves them to be 
different. Because thin dark, blackish-grey strata alternate with light 
ones that are rich in quartz, the folding can very distinetly be 
observed (fig. 2). The former are composed of closely compressed 
aggregates of light-green sericite, as a consequence of the folding 
the laminae were likewise bent. Little flakes of brown iron-ore (timonite) 
are abundantly spread. The lighter strata chiefly consist of aggregates 
of quartz, containing very few fluid inclusions. Further light greenish 
mica-lamellae are discerned, floating as it were in the quartzmass 
that is as clear as water. In other phyllites, besides grains of ore, 
many particles of carbon are spread and further prisms of tourmaline 
and needles of rutile. 

At the foot of Sangeang, situated on the upper-course of the Wai 
Miha, oceurs a black phyllite containing numerous hexaedrons of 
pyrite having a diameter of 2 mm., it has great resemblance with 
the rock collected by R. D. M. Verserk on the north coast in the 
neighbourhood of Cape Damar’). Under the microscope the eye 
distinguishes light strata containing much quartz, alternating with 
quite dark ones, which are filled with carbonaceous matter in sucha 
way that even the thin sections remain in some places opaque. It 
appears that the grains of quartz contain few and small fluid-inelu- 
sions. The rock moreover contains light-greenish laminae of sericite, 
needles. of rutile and 

If the quartz predominates a phyllitequartzite is formed. 

A similar rock is likewise found as a rock near the Wai Miha 


along the fissures — particles of limonite. 


and consists chiefly of whitish-grey quartz of a greasy appearance, 
interwoven with strata of phyllite. At last there is still a bowlder- 
phyllite in itself normal and containing small boulders of white 
quartzite and of siliceous limestone. The rock forms a counterpart 
of the boulder-clay slate described by E. KaLkwosky’). 

Near the upper course of the Wai Miha was found, besides the 
rocks described above, a waterworn specimen of clay slate which 
is strongly folded and apparently belongs to the same system of 
strata as phyllite. Microscopically it behaves as a common rooting- 
slate, contains as the latter numerous needles of rutile, a few prisms 
of tourmaline, and black widely distributed carbonaceous matter. 


1) Molukken-Verslag, p. 223. 
2) Uber Gerdllthonschiefer glacialen Ursprungs im Kulm des Frankenwaldes 
Zeitschr. d. D. geolog. Ges. 45. 1893, p. 69—86. 


256 


Van Novnvys moreover collected in the bed of the Wai Miha a 
phiyllite-breccia consisting of numerous angular, sometimes a little 
rounded fragments of phyllite having a diameter of at the utmost 
3 cm. They are usually strongly altered, and have consequently 
given occasion to the formation of chloritic minerals. As appears from 
the microscopic examination the white quartz-cement is composed 
of some grains of quartz as clear as water, the angles of which 
engage into one another like teeth. 

In the neighbourhood of Cape Pasturi boulders were found of a 
hard, grey, distinctly strated quartzite, containing moreover a great 
number of small hexaedrons of pyrite. Under the microscope the 
eye discovers, beside the grains of quartz which are as clear as 
water, green lamellae of chlorite, little titanite and a few black 
erains of ore. 

For the present moment it is still impossible to determine the 
age of the strata of phyllite. It is certain that the folding they have 
been submitted to, has taken place before the deposit of the Jurassic 
sediments which show nothing of this nature. Petrographically some 
fragments are completely identical to some Cambrian rocks in the 
Ardennes, especially those belonging to the etage devillo-revinien. 
Much nearer to hand is a comparison with similar rocks of the 
continent of Australia. Whilst there the Cambrian sediments are 
chiefly represented by limestones, those of the Praecambrium contain 
not only similar rocks as those of Taliabu, but it appears that they 
are likewise strongly folded all over the continent. 

In the strata of the Jurassic system found in Taliabu, a few rocks 
are found which, also from a petrographical point of view, draw 
special attention. Van Novunvys reported already that S. E. from the 
mouth of the Wai Najo cliffs are found consisting of “iron-hard 
“dark rock having on the fracture entirely the appearance of con- 
“olutinated gun-powder. This reck contains belemnites, which are 
“however as a rule badly conserved, and are often cemented with 
“the inclosing rock. Moreover the rock behaves entirely like granite, 
“as it is split into steep perpendicular prisms divided into blocks 
“by cross-fissures. This rock likewise changes into another of a 
“lighter colour, in which on the weathering-planes reddish quartz- 
“orains are found.” *) 

The rock that is meant here, is a chloritic iron-odlite (chamosite) 
dull, of a deep blackish-green colour, and containing numerous 
small grains, which have indeed great resemblance with gun-powder. 


1) Bydrage tot de kennis van het eiland Tahaboe, p. 1195. 


237 


As the colour makes us already suspect, in the thin sections under 
the microscope it is to be observed, that the rock is chiefly composed 
of fine dirty-green chloritie particles, which have been altered in 
the same way as those of the Chamoson-valley’). They contain a 
fine black dustlike matter, furtber pretty large grains of ore and 
moreover a few angular splinters of quartz. Some cavities are filled 
with erystals of calcite. 

As to the odlite-formations they distinguish themselves only from 
the other mass of rock by their structure. In the thin sections they 
are always of an elliptical or circular shape (diameter 0.08—0.6mm.) 
and consist of very thin green successive coats. The nucleus usually 
consists of a stranger body, as a rule of quartz, the grain of which 
occasionally becomes comparatively large (fig. 3). Though its shape 
may be ever so irregular the coats of the chamosite are always 


arranged in such a way that the unevennesses disappear, and the 
result is in the end a regular odlitic body. There are however 
likewise fragments of quartz in which every trace of a chamosite- 
edge is wanting. Exceptionally the fragment of the skeleton of a 
sponge serves as nucleus of an odlite. In consequence of an altera- 
tion the odlites change into a yellow- to red-brown mass. 
Formations of chamosite were also met with in other Jurassic 
sediments of the Najo-region. As van Nounvys has already remarked 
the chamosite-rock changes into another rock of a lighter colour ‘in 
which on the weathering-planes reddish quartz-grains are found”. 
The rock meant here, is a rather course sandstone, the quartz-grains 
of which have a diameter of 2 mm. The cement is of a greyish- 
green colour and effervesces strongly by treatment with hydrochloric 
acid. In thin sections one consequently perceives much calcite, partly 
in the shape of grains, in which the rhomboedrical cleavage is very 
obvious, for the greater part however in that of a fine scalish mass 
forming the real cement. The green chamosite is spread as in the 
above mentioned rocks, but odlites are only met with as a great 


1) G.Scummr. Ueber die Mineralien der Kisenoolithe an der Windgille im Canton 
Uri. Zeitschr. f. Krystallographie. XI. 1886, p.598. — Geologisch-petrographische 
Mittheilungen. Neues Jahrb, f. Miner, Beil. Bd. 4. 1886, p. 395. 


238 


exception. Parts of the skeletons of sponges have also been changed 
into chamosite in these rocks. 

Another sandstone of the same finding-place is more compact 
and contains much less calcite. Microscopically it appears to consist 
of angular and rounded quartz-grains, the intervening spaces of which 
are filled with fragments of sponges, the skeleton parts of which 
have been altered into chamosite. Odlitic formations are scarce. 

In connection with the rocks described above attention must 
be paid to a Limestone that was found in the Wai Najo in bank- 
shaped flakes. The greenish grey fine-grained rock leaves at the 
solution in hydrochloric acid a green sandy residue which appears 
{o consist of quartz and chamosite, the latter at the same time as 
petrifaction-material of numerous skeletons of sponges. In the thin 
sections of the rock the grains of calcite show rhomboedrical cleavage 
and form partly also polysynthetic twins. They likewise enclose 
particles of chamosite. Odlitie formations are not rare, but in this 
case only the outer zone consists of chamosite, whilst the inner 
part is still caleite, in which the rhomboedric cleavage-planes of 
the neighbouring grains of calcite have found their immediate con- 
tinuation, so that they form with these one individual. The skeletons 
of the sponges have been metamorphosed into pure green chamosite, 
whilst the intervening spaces are filled with limpid calcite. Besides 
ihe constituents mentioned numerous quartz-grains are present. From 
the above it appears that the limestone contains the same constituents 
as the sandstones that contain chamosite, and that there exists only 
a quantitative difference. 

As regards the formation of odlites, there can be no doubt that 
they have come into existence in the still soft mass of rock during 
or after the sedimentation. In my opinion they have originally con- 
sisted of carbonate of lime. That chamosite is no original mineral 
is already proved by the metamorphosed parts of the skeletons of 
sponges. It remains still unexplained which chemical processes have 
operated to bring this metamorphosis about. E. R. Zarinski has given 
an excellent summary of the different theories regarding the formation 
of thuringite and chamosite'), but it appears that none can be regarded 
as valid. 

Finally a few annotations about crystallized minerals of Taliabu 
may follow: 

Pyrite occurs — as has already been mentioned — in the shape 


‘') Untersuchungen tiber Thuringit und Chamosit aus Thiiringen und Umgebung. 
Neues Jahrb. f. Miner. Beil. Bd. 19. 1904, p. 79—82. 


239 


of cubic crystals in phyllites and quartzites of the Wai Miha region, 
whence also pseudomorploses of limonite originate. 

Quartz was found in limpid and dull-white crystals, attaining a 
length of 9 cm., found near Pela, situated between the Wai Miha 
and the Wai Ha. The shapes are the usual combinations of xf, 
Rand — R. 

Calcite. Elegant skalenhedrons 3 were found in a concretion, 
originating from the river Kempa, a tributary of the river Wai 
Miba, and likewise in a cavity of a geode with Macrocephalites. 
Small rhombohedrons are present in the cavity of the chamosite-rock 
in the neighbourhood of the mouth of the Wai Najo. 

Rhodochrosite occurs in the shape of small rhombohedrons on the 
walls of the air-chambers of a Macrocephalites from the Betino. 

Siderite was detected in a boulder of quartzite, originating from 
the upper-course of the Wai Miha, in the shape of yellowish rhom- 
tbohedrons. Brown rhombohedrons together with calcite were found 
in the chambers of an Ammonite from the Wai Galo. 

Barite. All the chambers of Macracephalites keewwenis G. Bown 
are sometimes filled with limpid barite in such a way that the 
whole mass forms one individual. 


Chemistry. — ‘Studies in the Field of Silicate-Chemistry.” 1. 
On the Lithiumaluminiumsilicates whose composition corresponds 
to that of the Minerals Eucryptite and Spodumene. By Prof. 


F. M. Jancer and Dr. Anr. Stwek. (Communicated by Prof. 
P. van RompBurGH). 
(Communicated in the meejing of May 30, 1914). 


§ 1. In connection with the study of the ternary system, whose 
components are: Lithiwmovide, alumina and silica, it was necessary 
for us, to obtain the compounds, whose composition corresponds 
with that of the minerals ewcryptite and spodumene, in a perfectly 
pure state, and to investigate their characteristic properties. The 
third ternary compound, corresponding in its Composition with the 
mineral petalite, will be taken in account only afterwards, as for some 
reasons it is better to deal with it, when the experimental study of 
the ternary mixtures themselves shall have proceeded some-what further. 

The eucryptite: LiAlSiO, belongs to the series of silicates, whose 
other members are: nepheline, kaliophilite, ete. In nature the said 
compound occurs in the form of microscopical, hexagonal crystals, e. g. 
in the albite of Brancnmvittn (Conn.) ; albite and eucryptite both take 
their origin here from spodumene, decomposed by solving agents. 


240 


The spodumene LiAlSi,O, is a monoclinic lithiumpyroxene. The 
mineral is found in several places, in the form of colourless or feebly 
tinged, glassy crystals of prismatic habitus, or in the form of opaque, 
eryptocrystalline aggregations. The transparent or coloured varieties, 
which are strongly dichroitic, are used as a beloved precious stone ; 
they are: called: triphane, kunzite, hiddenite, ete. Their properties are 
mentioned further on. 


§ 2. As was already pointed out, in a previous paper *) on 
lithiumsilicates, the synthesis of the pure compounds offered severe 
difficulties, caused by the volatilibility of the lithiumoxide at higher 
temperatures. The composition of the mixture is thus altered during 
the synthesis, and the quantities of all three components must there- 
fore afterwards be corrected, after being accurately determined by long 
and troublesome analysis. A relatively small loss of the lithiumoxide, 
is of considerable influence on the meltingpoint and other properties 
of the investigated compound, because of the very small molecular 
weight of the oxide. The analysis offered many difficulties: for 
notwithstanding all care and all arrangements’), it often happens, 
that some A/,O, is found in the silica, and some SO, in alumina, 
so that afterwards a controlling determination of these admixtures 
must be made, which takes a lot of time. The small amount 
of Li,O is furthermore hardly determinable under the colossal excess 
of Na,O in the liquid; therefore, being determined as the difference 
of 100°/, with the sum of the percentages for S’O, and A/,O,, all 
mistakes and inaccuracies of those determinations are summed up in 
the number for L7,0, so that the correction of the preparation after- 
wards, often depending on very slight differences in the amount of 
Li,OQ, is a hazardous and not very amusing task. So it takes much 
time to obtain products, which will not differ appreciably im their 
constants and properties from those to be expected for the true pure 
compounds, the criterium being given by the perfect identity of the 
products, prepared in several ways. 


§ 3. Synthesis and Properties of the Pseudo-Kucryptite. 

The materials for this and other syntheses were the same, 
whose purity was before tested and described; the alumina used 
was also provided by Bakrr and ApaAmson. It was necessary to heat it for 
a long time in a platinum dish on the blaze, and often to stir the 
powder with a platinum-wire, to allow the watervapour and the nitrous 
gases, which the preparation evolved, to escape completely. The 


1) FE. M. Jaeger and H. §. Knoosrer, these Proceedings p. 900, Febr. (1914). 


241 


heating was checked when the weight of the dish remained constant 
after repeated heatings. Analysis then showed, that an almost pure 
Al,O, (100°/,) was present; even no appreciable trace of iron could 
be demonstrated with the usual reagents. 

To point out the change of composition, taking place on heating 
mixtures of known composition during the melting of the mass, the 
numbers here following can serve very well: a mixture of 6,23 gram 
Li,CO,, 8,61 gram Al,O, and 10,16 gram SiO,, was melted in 
a closed platinum erucible in the Frrrcumr-furnace at 1500° C. 
After crystallisation, the mass was finely ground and sieved, melted 
again, and this process repeated three times. Instead of the expected 
composition /, the composition // was found by analysis to be: 


/ IT 
SiO, A7,7°/, 48,6°/, 
Al, 0, 40,4°/, 40,9°/, 
Oe 11,9°/, 10,5°/, 


As there was thus 1,5°/, Lz,O0 too little, 0,055 gram Al,O, 
and 0,718 gram dry Li,CO, were added to 18,92 gram of the 
resulting product, and this mixture was then heated four times in 
platinum crucibles, by means of small resistance-furnaces, at 900° or 
1000° C., the mass being finely ground and sieved after every 
melting. Then the preparation was again heated once at 1450°C. 
in a resistance-furnace. Analysis gave: 


Odserved : Calculated : 
SiO, 47,9°/, 47,7 °/, 
Al,0, 40,1 °/, 40,4°/, 
Li,O 12,0°/, 11,9°/, 


The deviation from the exact composition is so slighf, that this 
preparation could safely be used for the study of the properties of 
the compound, 


§ 4. The meltingpoint of this preparation was determined several 
times by means of a calibrated thermoelement (N°. ///). The mean 
value of all readings was 14200 M.V. + 2 M.V.; as the correction 
of this element with respect to the standardelement, which was 
standardized by means of Sosman’s element G, was -— 12 M.V.; 
the meltingpoint of the substance, in terms of the Washington nitro- 
vengasthermometerscale, can be fixed at 1888° C. 

The heat-effect on melting is only small; as a result of that, on 
cooling down the molten mass, one finds a retardation of its erystal- 
lisation up to about 12840 M. V.; then crystallisation takes place 
while the temperature increases only to 1306° C. The point of 


242 


solidification therefore is found 80° or 90° below the true tempe- 
rature of equilibrium: solid = liquid, although the velocity of crys- 
tallisation can by no means be called very small. From this faet 
also the discrepancies in the data of different authors are to be explained : 
1330° C. (Dirrier and Baio), 1807° C. (Ginsprre), etc. In this case 
also, the usual method of cooling appears to give no reliable results. 

A remarkable fact is the relatively appreciable cncrease of the 
volume of the molten mass on crystallisation; it is immediately 
observable by the deformation of the platinum-crucible. (fig. 1). That 
really this phenomenon is caused 
in this case by a volume-change like 
that of water into ice at the freezing- 
point, and that it need not be explai- 
= i. ned in the manner mentioned in the 


Fig. case of the spodumene, can be demon- 

Increase of the volume of molten ‘Strated by the determination’ of the 
Eueryptite on crystallisation. specitic gravities of the erystallized 
mass, and of that of the beautiful, colourless ‘glass’, obtained by 
suddenly chilling the liquid. The expansion seems to be about 3°/, 


of the original volume. 


§ 5. The crystallized substance, obtained by slowly cooling the 
liquid, is opaque and greyish white. Microscopical investigation 
showed it to be a eryptocrystalline aggregation of irregularly shaped, 
erain-like crystals, which are so small, that even with an 800-times 
enlargement, they can hardly be seen; they possess a very weak 
birefringence. Greater pieces seem to be built up between crossed 
nicols by innumerable lighting points ; such aggregations always show 
an undulatory extinction. In no case erystals with determinable 
borders were found. As a ‘mean’ refractive-index the value: 
Ny = 1,531 + 0,002 was obtained. 

The specific gravity at 13°,6 C. was pyenometrically found to be: 
do 2,365, and at 25°, C: dy = 2,362 ; we used orthochlorotoluene 
(1,0825 at 25°,1 ©.) as immersion-liquid. 

As follows clearly from those values for the refraction of light 
and for the specific gravity, the natural eweryptite must be another 
modification of the compound Lz AlSiO, ; therefore we will distinguish 
the artificial silicate by the name: pseudo-eucryptite. *). 


1) Ginspera (Zeits. f. anorg, Chem. 73. 291 (1911)) describes his preparation in 
the followmg manner: completely isotropous, uniaxial negative in convergent pola- 
vised light, with a birefringence smaller than that of nepheline. Weypera asserts 
to have obtained an “eueryptite” of rhombic symmetry, by the reaction of Li,SO, 
on kaoline in solution. Cf. also the experiments of Tuuaeurt, Zeits. f. anorg. Chemie 
2. 116. (1892). 


245 


§ 6. The glass, obtained by suddenly chilling the molten mass 
in mercury or cold water, is colourless, perfectly clear and exceed- 
ingly hard. It can be removed from the platinum-crucibles in an 
easier way than the crystallized mass, which fact is connected with 
the volume-change in crystallizing. 

The refractive index of the glass appeared to be: mp) = 1,541. 
We have prepared several glasses of varying chemical composition, 
all in the vicinity of the composition of the pure compound, with 
the purpose to measure accurately the refractive indices and the 
dispersion, in order to get information about the influence of the 
chemical composition on the optical behaviour of these glasses. They 
were ground in <a flat cylindrical form, and in all directions care- 
fully polished; then they were investigated by means of an ABBE- 
erystalrefractometer in light of different wave-lengths. 

For pure pseudo-eucryptite-glass of the composition LiAlO,, 
we found: 


Wavelength in A\.U. Angle of Total- Refractive A: 


reflection : Index : 

Ii: 6708 62am 1.5450 
0,0040 

Na: 5893 61°54’ 15410 
0.0056 

Sips 5350 Olson 1,5354 


In the following are summarized the measurements with the glasses : 
LT. Compos: 47,5°/, Si O,; 40,0°/, Al, O; ; 2 Dif ta), 


HEE Compos: 42°55), Su Onc 30:0° (Al O, > 18,99 /5 ha. C). 
i VesCompos:, 48.4°/- S71 Obs 39:39), Al. 0, > 1 i RO! 
Gt. 
Wavelength in Angle of Refractive Ne 
eet Oe Totalrejlection : Index: 
Li 6708 62°26’ 1,5484 
0,0047 
Na 5893 G2ebr ie 1.5437 
| 0,0044 
Tl 5850 61°47’ 1,5395 
LUE 
Wavelength in Angle of Refractive aN 
INGE dee Totalrejlection : Index : 
li 6708 63°36" 1.5647 
0,0048 
Na 5893 Gave 1.5599 
0,0039 


fl 5390 62°58’ 1,5560 


244 


LV 
Wavelength in Angle of Refractive A: 

ICE Oa Totalrejlection : Index: 

li 6708 61°50’ 1,5400 
0,0046 

Na 5893 61°31’ 1,5354 
0,0053 

fh) 5350 Gie97 1,53801 


It is difficult to deduce a simple relation of chemical composition 
and optical properties from these data. Generally speaking, an 
increase of the amount of 7,0 seems to cause an_ increase 
of the refractive power (except in JV), while a larger amount . 
of SO, appears just to diminish the refractive index, the exceptional 
case /V could be explained by the superposition of these two causes. 
This dependence of the quantities of the oxides present, appears to 
bear some connection with the relatively higher refractive power of 
the lithiumoxide, and the smaller one of the silica '). 

The pseudoeucryptite-glass is, with respect to the opaque, erystal- 
lized compound, a typical metastable phase: already on heating the 
glass during a very short time in a Bunsen-gasburner, the pieces of 
glass become primarily yellowish, then they become opaque, 
and finally they appear under the microscope wholly changed into 
the mentioned cryptocrystalline aggregation of birefringent grains. 
If heated only for ten minutes at 900°C., they are completely - 
changed, and the same occurs, on heating the finely powdered glass 
during some time with molten LiCl or LiF in a platinum crucible. 

The specific gravity of the pare pseudo-eucryptite-glass was deter- 
mined by means of the method of swimming, in a mixture of 
bromoform and benzene, at 13° C.; it was found to be : dy = 2,429. 
Thus both the refractive index and the density of the glass are 
somewhat higher than for the crystallized compound. 


§ 7. Finally we have compared the artificial product with a 
natural eueryptite of BrancunviLLe (Conn.). The mineral, of which 
a thin section was prepared, looked as an aggregation of erypto- 
crystalline, homogeneously extinguishing fields: however, although 
they had superficially some analogy with the artificial product, they 
must be considered as composed of much larger crystals, showing 
apparently the kind of structure, somewhat similar to the so-called 
“schrift”-granite. Locally it is intermixed with a much more strongly 


1) fF, M. Janeen and H. S. van Kuoosrer, these Proceedings, loco cit. (1914). 


245 


birefringent mineral; although the eucryptite is here generated from 
spodume. with deposition of albite, the properties of the inclusions 
did not agree with those of the two lastnamed minerals. The 
specific gravity was pycnometrically determined to be dyo = 2,667 
at 25°C.; the available data show the composition not to be the 


proper one, the S’O,-amount being 0,6°/, too high and that of the 


LiV,z about 1°/, less than the theoretical value. The fig. 2 and 3 
represent two microscopical preparations of the thin section between 
erossed nicols; in the fig. 3 the preparation is turned over 30° with 
respect to that in fig. 2; — this fact pointing to a trigonal twinfor- 
mation. Also the very peculiar structure of the crystals is shown 
in fig. 3. 

The refractive index was microscopically determined on : 2p = 1,545 
+ 0,002. A definite meltingpoint could not be fixed by the usual, 


1 


dynamical method; at about 1120° C. the mineral gradually changes 
into a viscous mass, which, on cooling, becomes a glass. The refrac- 
tive index of this glass appeared to be: np=1,506 + 0,001, it is 
thus evidently lower than that for the glass of psewdo-eucryptite. 
On being heated it is devitrified only slightly; there seems to be no 
doubt, that the natural mineral and its glass are other than the 
corresponding phases of the artificial product. As also never any 
indication of an oceurring inversion could be found, it is highly 
probable that eucryptite and pseudo-eucryptite are in relation of 
monotropic modifications to each other. 


§ 8. Synthesis and properties of (?-Spodumene. 

The compound, ~ whose composition is: LiAlS7,0, was prepared 
17 

Proceedings Royal Acad. Amsterdam. Vol. X VIL. 


246 


by us in four different ways, just to get information on the final 
identity of such preparations: 

a. By melting together calculated quantities of Li,CO,, Al,O, and 
SiOQ,, repeating this manipulation a few times, after thoroughly 
erinding and sieving the crystallized masses. Analysis and correction 
were made as usual. 

b. By starting from pure Lz,S70,, Al,O, and SiO,. 

ce. From LiAlSiO, and Si). 

d. From LiA/O,, the lithiumaluminate, and S7O,. 

The four preparations, thus obtained, were used only for the 
definitive measurements after it had been proved by repeated ana- 


2? 


lysis and correction, that their composition did correspond, within 
the limits of error, with that of the formula. AIl these experiments 
were made in electrically heated furnaces with oxidizing atmosphere ; 
the preparation of these substances took a long time, because of 
the volatibility of the 7,0, and the fact, that only small devia- 
tions in the content of 7,0 showed themselves of appreciable 
influence on the meltingpoint and properties of the compound. 


§ 9. The purest preparation we got, was obtained from  synthe- 
tical eueryptite by admixture of SvO,. Analysis gave the following data: 
I. 1 Caleulated : 
SiO, 64,39 °/, 64,438 °/, 64,6 °/, 
AlsOe 227,000), 27,66 °/, 27,4 °/, 
I1,O 8,05 °/, ieoies 80°75 
The mass was kept during a longer time at a high temperature, 
to allow it to erystallize totally. Then the meltingpoint was deter- 
mined in the usual way, by means of thermoelement ///; we found : 
14353 M. V. 
14341 MM. V. 
Mean: 14347 J/. V. (without correction), 
if the rate of heating was about 65 M.V. pro minute. As the correction 
for the thermoelement was — 12 M. V. at this temperature, the 
meltingtemperature is 1400°C., in terms of the nitrogenthermometer. 
As a check the mellingpoint was now again determined by the 
statical method: very small quantities, wrapped in platinum folium 
were heated during a considerable time (from half an hour to one full 
hour) at a certain and accurately constant temperature, and then, 
after suddenly chilling *) in cold mereury, investigated by means of 
1) F. M. Jareer, Kine Anleitung zur Ausfiihrung exakter physiko-chemischer 
Messungen bei héheren Temperaturen. Groningen, 1913, Seite 73, 74. 


947 


the’microscope. We found that after heating at 14340 M. V. (element IIT) 
the whole preparation was again crystalline, although it had the 
outward appearance of a glassy, half-opaque mass; but on heating 
at 14360 M. V., all had been changed into a real “glass”. The 
meltingtemperature therefore must be fixed at 14850 M. V. As the 
correction for the used quenching-system (vid. the determinations of 
the meltingpoint of natural spodumene of J/adagascar) was shown 
to be practically equal to zero, we can conclude from this, that the 
meltingpoint thus determined is in full agreement with that found 
by the dynamical method, and can be put at 1401°C.(G Th.). The 
crystallized product appeared to be identical with the /?-modification, 
later to be described, the refractive index was about: » = 1,521; 
the specific gravity at 25° C: dy = 2,411. 

2. In a similar way the preparation, obtained from lithinmaluminate 
and SiO, was investigated; analysis gave the following data: 


I Il Calculated: 
StO, 64,80°/, 64,07°/,  64,6°/, 
AGO 2S Os fae 205092 2 e 
Li, O Cpa edie a liptess sali 8,0°/, 


This preparation therefore evidently can also be considered as a very 
good one; it contains ca. 0,4°/, 17,0 too little, and ca. 0,5"), Al, O, 
too much. 


Fig. 4. 
Artificial 6-spodumene, obtained from LiA/O, 
and Si0,; melted and slowly cooled. 


CX Nicols). 


248 


The meltingpoint, determined after the dynamical method (element 
IT]), was found: 
14463 M. V. 
14481 M. V. 


Mean 14472 M. V. = 10 M. V. (without correction) ; 
after correction, the meltingpoint can be fixed at 1410° + 1° C. (G.Th.). 
After the statical method, the meltingpoint was determined at 
14450 M. V., corresponding to 1410°C. The small excess of A/,O, 
has evidently caused an ncrease of the meltingtemperature, of about 
9°C. The erystallized product again was shown to be /?-spodumene 
(n= 1,519); a photograph of it, taken between crossed nicols is 
reproduced in fig. 4. 

3. An analogous result was, in both ways, obtained with a pre- 
paration, prepared from Li,S/0,, Al,O, and SvO,. Analysis of this 
product gave the following data: 

] II Caleulated : 
SiO, 64,7°/, 64,48°/, 64,6°/, 
Al,O, 28,4 °/, 28599) 2a ye 
1,0 G95 Ce S076 

The content of S/O, is here the right one, but the Ad,O, is 1°/, 
too high. The meltingpoint determinations gave as a mean value: 
14456 M.V. (uncorr.) after the dynamical method, and about: 14450 
M. V. after the statical method. The meltingpoint is therefore : 
11092 (Ch(Gelhe): 

4. Most deviating from the composition: Li AlSi,O,,. was a pre- 
paration, obtained from the melting together of £7,C0,, SiO, and 
Al,O,. Analysis gave the following numbers: 

I II Caleulated ; 
SiO, 64,44°/, 64,88°/, 64,6°/, 
Al.O,, J2T09/. SEAT Uh eno Ane 
Li,0 —*847 > S795 eS Sey) 

Evidently it contains about 0,21 °/, Z7,0 too mueh. 

After the first method the meltingpoint was found at 14552 M.V. 
(uneorr.), and after the statical method: 14550 M.V. The true melting- 
point can thus be put at: 1417° C. (G.Th.). 


§ 10. Although in most eases perfectly colourless products were 
obtained, which evidently were identical to and independent of the 
particular manner of preparing them, and which all represented the 
8-modification, —- we succeeded however in several cases in obtaining 
beautifully erystallized preparations, which locally or also totally were 


249 


tinged with a nice, reddish lilac hue; they were in most cases 
obtained by longer heating, somewhat below the meltingtemperature. 

The meltingpointdetermination with such an intensively coloured 
product, prepared from L7A/O, and SiO, and showing by analysis 
the following composition : 

I. Me Caleulated : 
S72, 64-92) o)s NEARY. F< Gd6/5 
Al,O, 28,10°/, 27,94°/, 27,4 °/, 
ROTC OSS 29) SOR 
and thus evidently containing about 0,68°/, too much alumina, gave 
the following results (statical method) : 
After heating at 14660 M. V.: all glass. 
14640 M. V.: all glass. 
14600 M. V.: all glass. 
14500 M. V.: all erystallized. 
14560 M. V.: all crystallized. 

The meltingpoint is thus situated at 14580 M.V., corresponding 
with 1420° ©. (G.Th.). 

Such lilac coloured preparations present in most cases rather 
larger individuals of the 2-modification, which possess a tabular shape 
with appreciably stronger birefringence than the common erypto- 
crystalline masses, although the mean refractive index is the same. 
While commonly this birefringence varies between 0,001 and 0,008, 
it amounts in these preparations to about 0,007 ; the principal refrac- 
tive indices are about: 1,520 and 1,527. In convergent polarized 
light, at the border of the field an interference-image is partially 
visible, giving the impression of that of an uniaxial crystal. However 
on moving the table of the microscope, one can easily observe the 
curvature and even the hyperbolic form of the dark beams; undoubtedly 
an optically biaxial erystal with a very small axial angle, is present 
here; while the position of the first bisectrix and the character 
of the dispersion, point to monoclinic symmetry, with a strong 
tendency to tetragonal forms. This last pecularity can be deduced, 
— besides from the apparent uniaxity — from the fact, that rectangular 
plates are not rare, which possess an extinction under right angles 
or parallel to a diagonal, and a system of cleavage-directions under 
45° with the optical sections. The specific gravity, like the refractive 
indices, does not differ appreciably from that of the common @-form, 
and was determined at 25° C.: d» = 2,401 + 0,008, measured with 
several preparations. We obtained these same apparently uniaxial 
plates, also from natural spodumenes by melting and slowly crystal- 
lizing; there is no doubt whatever about the fact, that these tabular 


250 


crystals are identical with the common g-form, which represents 
the stable form at the meltingpoint; the plates must be a peculiar 
kind of erystals of this g-modification. 

However we have till now not succeeded in giving a final explan- 
ation of the remarkable reddish-lilac colour of many of these pre- 
parations. It is quite sure, that it does not depend in any way on 
the admixture of certain metallic impurities, solved from the crucible- 
walls; on the contrary it appears to be connected with the macro- 
crystalline strueture of the preparations. The nearer the chemical 
composition came to the theoretical one, and the slower the crystal- 
lisation of the mass takes place, by heating during a long time at 
a temperature just below the meltingpoint, the more the appearance 
of the violet tinge seems to be probable. 

The same colour appears, if spodumene-powder or the pulverized 
“glass” of it, are brought into liquids of about the same refractive 
index (e. g. inta orthochlorotoluene, with n= 1,522); in that ease 
the wellknown phenomenon of the “monochromes” (CHRISTIANSEN) 
will appear. It is not impossible, that in our case the colour is 
produced in An analogous way by the presence of the tabular, very 
thin crystals amidst spodumene-glass, which possesses about the 
same refractive index (1,519) as the ecrystal-tables (1,520 till 1,527), 
or Yeversely ; these tables would be therefore quite invisible in the 
surrounding medium. It could be understood in this way also, why 
in the uncoloured mass in some cases locally smaller or larger 
pink spherolithes are produced, making the impression, as the molten 
mass were locally inoculated with germs of the violet substance. 

By means of the ultra-microscope we were able to show, that the 
preparation was not “optically empty”, as a great number of differ- 
ently coloured lightspots, which do not move however, could be 
observed; they are manifesting a structure of some particular kind, 
without it being possible to ascertain of what kind the imbedded 
particles are. 

§ 11. As it follows from these investigations, in connection with the 
meltingpoint determinations of natural a-spodumene later to be described, 
that the chemically pure compound LiAlSi,0, has a meltingpoint 
considerably lower than the natural spodumene-minerals, — we made 
a series of investigations to find out, what admixtures of the natural 
spodumenes might canse the mentioned increase of the meltingpoint. 
Therefore to an artificial product, whose composition was: 

StOp Ie oder 
ALO; Dida fe 
Li,O 8,2) /6 


we added successively in concentrations of 1 mol. percentage, the 
following chemically pure preparations : 
Observed and reduced 
Meltingpoints: 


1. Jadeite: NaAlSi,O,, synthetical. elas SMe —— 382° 
2. Leucite: KALSi,O,, synthetical, anhydrous. 14506 M.V. = 1414° 
3. Lithtwmowide: Li,O. 14304 M:V. = 1397° 
4. Alumina: Al,O,. 14585 M.V. = 1420° 
5. Silica: SiO, (quartz). | 14530 M.V. = 1416° 
And in concentrations of 2 mol. pere.: | 

6. Pseudowollastonite: CaSiO,, sy nthetical, 14357 M.V. = 1402° 
7. Siliimannite: Al,SiO,, synthetical. 14593 M.V.=1421° 


Keeping in mind, that the pure substance melts at 1417° C. 
(G. Th.), we can deduce from these experiments, that : 

a. An excess of L7,0 lowers the meltingpoint of the compound 
LiAlSi,O,, while the influence of an excess of S’O, is somewhat 
uncertain, but seems to produce a slight increase. 

b. That a lowering of the meltingpoint is also produced by an 
excess of synthetical jadeite, leucite and pseudowollastonite, which can 
be considered as the principal admixtures of the natural kunzites 
and spodumenes. 

c. That on the contrary, an dncrease of the meltingpoint is produced 
by an excess of alumina and of alumosilicates, like e.g. pure 
sillimannite. 

In how far these facts, which of course will be studied more in 
detail, when the ternary system: Li, 0—A/,O,—Si0, is investigated 
completely, can be used for the explanation of the phenomena, 
observed in the case of the natural spodumenes, will be shown in the 
next paper. 

Groningen, May 1914. Laboratory of Inorganic Chemistry 

of the University. 


Chemistry. — ‘Studies in the Field of Silicate-Chemistry. UL. On 
the Lithiumaluminiumsilicates, whose composition corresponds 
to that of the Minerals Eucryptite and Spodumene”. By 
Prof. Dr. F. M. Janeer and Dr. Ant. Smek. ( Continued ). 
(Communicated by Prof. P. van Rompureu.) 


(Communicated in the meeting of May 30, 1914). 


§ 12. For the purpose of comparison of the properties of the 
described artificial product with the mineral itself, we have inves- 
tigated a number of natural spodwmene-species in an analogous way. 


252 


We obtained a number of very pure funzites, and some good 
spodumenes: 

1. An almost colourless, somewhat lac tinged, strongly dichroitie 
kunzite from Rincon in California. 

2. A completely transparent, glassy, pale rose tinged kunzite from 
Suhatany-valley on Madagascar. 

3. <A beautiful, transparent pale greenish yellow kunzite from 
Minas Geraés in Brasil. 

4. A transparent, emerald-green hiddenite from Alewander County in 
North Carolina, U.S.A., anda pale yellow hiddenite of the same place. 

5. A eryptocrystalline, opaque piece of spodumene from Somerd, 
in Finland. 

6 An aggregation of opaque, long prisms of spodumene from 
Maine, U: oh A. 

All meltingpoints of the finely ground material were determined 
in exactly the same way and with the same care, as formerly 
described. The specitie gravities were determined by means of a 
pycnometer, with ortho-chlorotoluene as an immersion-liquid; the 
oravity of this was: dy = 17,0841 at 25°,1 C. 

Most of the optical data were obtained by microscopical investi- 
gation; the values of the refractive indices are determined at 16° 
oye AY (Ce 


specific 


1. Kunzite of Rincon, Cahfornia. 
Big, very feeble lilac colours, very lustrous and perfectly trans- 
parent crystals, evidently with a cleavage parallel to the vertical prism. 
An analysis of Davis, made with the same material, gave the 
following results : 
Calculated: Impurities : 

70. : 64,05°%/ - 64,64), CaO R10; Sif: MnO : 0,11°/, 
A,O, : 27,30°, 27,45, Na,0:03 °°,  NeOmmomegn 
TOO 388.5) S01. ZnO: 0,44°/, K,O : 0106 

Total: 0.78 °/,. 

The crystals show a strong fluorescence under the influence of 

RONTGEN-rays. 


The meltingpoint determinations gave, with thermoelement IV, the 
following results: as a mean value of a greater number of obser- 
vations, we found: 14683 M. V. + 4M. V.; as the correction of the 
thermoelement at this temperature was — 8M.V., the melting-point 
is thus: 1428° C. (G. Th.). It is very sharply localised on the 
heating-curves. 


253 


The specifie gravity at 25,1° C. was: dy = 3.204 + 0,008 for the 
natural, not yet melted compound; after solidification of the molten 
mass, one obtains, after slowly cooling, a colourless, finely crystal- 
lized mass, whose density differs considerably from the original mineral; 
itis dqi==92, cor a 2o>,1aC. 

The refractive indices of the molten and solidified substance are 
considerably different from those of the original mineral. While tor 
the unmelted substance we found respectively: 2, = 1,658 + 0,008; 
— ARGE9H= = O1O03 Zande rie —1nGi-2) = 01003 2) for: the solidified 
mass we found an extremely feeble birefringence of about 0,001, 
and a mean refractive index of: 2p —= 1,518. The erystalpieces showed 
an irregular extinction, evidently by very complicated intergrowth 
of several individuals. 

On rapidly cooling, an isotropous glass was obtained, with a 
refractive index of m, = 1,517 + 0,001, being about the same as 
for the crystallized mass. The specific gravity was at 25°,2 C.: 
d,o = 2,388 + 0,003. When heated during a longer time at 1300° ©., 
it becomes erystalline; even at lower temperatures the glass gets 
soon opaque and like porcelain by devitrification; but glass and 
crystalline product obtained from it, evidently do not differ in their 
properties to any appreciable amount. 


Il. Kunzite of the Sahatany-valley on Madagascar. Big, clear and 
completely transparent crystals; they are dichroitie and tinged with 
a pale rose hue. Locally the environing rock-material is again 
discernible, as a rusty coloured, finely divided substance. The erystals 
were carefully cleaned from it; then they were ground and sieved, 
after which the investigation proceeded in the usual manner. 

As a mean value for a greater number of determinations, we 
found the meltingpoint at: 14683 +5 M.V.; as the correction of 
the thermoelement was —8M.V. at this temperature, we can adopt 
the value 14675 M.V. of the E.M.F. of the thermoelement at the 
ineltingpoint, corresponding with: 1428° C. (G. Th.); in this case 
the meltingpoint is also very sharp. 

Evidently this kunzite differs only slightly from the preceding 
mineral of Rincon. With respect to its chemical composition, we 
have some data, given by Lacroix’), who investigated colourless, 

1) In a liquid of nm» = 1,670, composed of methylene-iodide and monobromo- 
naphtaline, the crystalpowder showed a very beautiful reddish-violet colour, just as 
some of CuristIANsen’s “monochromes”. The same phenomenon was observed fo1 
the glass and the @-modification of artificial spodumene. 

2) A. Lacroix, Minéralogie de la France et ses Colonies, [V, 775, (1910). 


254 


greenish-yellow and rose kunzites (triphane) from Maharitra on 
Madagascar; the lilac and rose kunzites of Ampasihatra are im- 
bedded in a kind of kaoline-earth, generated from the spodumene 
by decaying-processes. The green kunzites possess the greatest values 
of their refractive indices, however only little differing from the 
other ones, while the rose tinged erystals have a smaller, the colour- 
less ones yet smaller values for those constants. 

We found by means of the immersion-method n, = 1,658 and 
n, = 1,673, which values do not differ appreciably from the mean 
values: n, = 1,6588, n, =1,6645 and n, = 1,6750.') For the ana- 
lysis of the red and greenish crystals, the following data are given 
in literature; they are reproduced here for comparison with the 
composition of the Californian kunzite : 

rose cristals: | green cristals: 
SiOz :63,85% 9 CaO : 0,529) MnO : trace | SiO, :62,21%9 CaO :0,50% MnO : trace 
AlyOy:29,87%\y NagO: 0,98) Fe,03:0,15%) | AlzO3:29,79%) NaO: 1,03%y) Fe03: 2,489/g 
Li0 : 3,76%9 MgO :0,13°%/9 KoO :0,13%p Li,O : 4,02", MgO : trace K,O  :0,212%p 
Residue : 0,37%. | Residue: 0,25%p. 

From these data results, that the quantity of S’O, in the rose 
crystals is about the same as for the pale rose kunzite of Rincon; 
but the content of A/,O, is much greater in the mineral of Mada- 
gascar, and thus the 2,0 appreciably less than in the American 
kunzite. The sum of those three constituents does not differ very 
much in all these cases: 97,5°/, for the kunzite of Madagascar, 
95,2°/, for that from Rincon. The specific gravity of the rose species 
is about 3177: a value, only slightly different from the value, 
determined by us: d,e = 38,3801 + 0,005, at 25°,1 C. 

The refractive indices of the melted, feebly birefringent produet, 


were found to be n, = 1,518 and n, = 1,520; the birefringence is 
not greater than 0,002. 

At 25°,1 ©. the specific gravity of the melted and solidified sub- 
stance was determined: d,° = 2,373, when the preparation was heated 
during several hours at a constant temperature, just below the 
meltingpoint; under the microscope the obtained product then showed 
the typical aspect of the aggregates of scales, which are always found 
with the @-spodumene; they have a weak birefringence, and an 
irregular, often undulatory extinction. When «-spodumene was not 
melted before, but only kept at a constant temperature below the 
meltingpoint, the substance appeared to be wholly transformed into 
the same @-modification, with a specific gravity of: do = 2,376 at 


1) Duparnc, Wunper et Sasor, Mém. de la Soc. physique de Geneve, 36, 402, 
(1910). 


259 


25°,1 C. In both cases the mean refractive index for sodiumlight 
was: ny = 1,518 + 0,001. From the molten mass therefore no other 
phase is deposited than the mentioned 8-modification. 

The fig. 5, 6, and 7 may give an impression of the manner, in 
which the transformation of the e-, into the /?-modification gradually 
occurs. In fig. 5 the original kunzite of J/adagascar is photographed 
between crossed nicols, when heated only during 2 hours at 975°C., 
and showing no trace yet of the @-form; in fig. 7 the same heating, 
but prolonged to 15 hours, has led to complete transformation of the 
erystals into the #-form. The fig. 6 represents the crystals, after 8 
hours heating at 975° C.; they show a partial transformation, and 
the gradually occurring differentiation of the originally homogeneous 
crystals into an aggregation of the felty needles of the @-modification. 

Ill. Greenish-yellow Kunzite of Minas Geraés, Brasil. 

This kunzite appears also in the form of large, very transparent 
crystals, having a pale greenish or yellowish hue. This colour is 
caused by a content of /eO, which in melting the mineral, is con- 
verted into: Fe,0,; thus the solidified mass being always tinged 
with a reddish-brown colour. The analysis of this mineral ') gave 
the following data : 


SiO, : 63,3— 64,3°/, CAOr 02-00 
Al,O,: 27,7—27,9°/, Na,O: 0,6—1,0 °/, 
1,0, : i 7,4°/, FeO ° O12 WE 


This kunzite therefore is also relatively close in composition to 
that of Rincon, approaching in its content of L7,0 closer to the 
theoretical value; the sum of the principal constituents is 97,7 °/,. 

The meltingpoint of this mineral was determined five times; the 
results were, with thermoelement IV: 


14643 M.V. 
14646 M.V. 
14650 M.V. 
14639 M.V. 
14646 M.V. 


Mean value: 14645 M.V.; 
after correction: 14637 M.V. (G. Th.) 
The meltingpoint, reduced on the nitrogengasthermometer, lies 
thus at 1425° C., i.e. about 3° C. lower than for the kunzite of Rincon. 
The specific gravity of the substance before melting, was deter- 
mined at 25°,1 C. to be: dy= 3,262; the data, given in literature 
for the specific gravity of natural crystals, vary between 3,16 and 


% 1) CG. Hintze, Handbuch der Mineralogie. 


3,174. The refractive indices of the original substance were: 2, = 1,661 
and n, = 1,669, with apparently a somewhat weaker birefringence 


as for the already deseribed kunzites. 


Fig. 5. Fig. 6. 
Kunzite of Madagascar, heated tor two hours Beginning of the transformation of z-spodumene 
at 960° CG. and not yet perceptibly transformed, (Madagascar), after being heated during eight hours 
(X Nicols). — - at 975° CG. (X Nicols). 


Fig. 7. 


Kunzite of Madagascar, completely transformed into 
the 6-form, after being heated at 975° C. (< Nicols). 


257 


After being melted however, the reddishbrown, crystalline product 
had _a specific gravity at 25°,1 C.: dy = 2,463, while the refractive 
indices of the feebly birefringent grains were found to be about 
1,522 and 1,527. There is no doubt whatever about the fact, that 
the solidified product is again a modification absolutely different from 
the original kunzite; moreover it is evidently identical with the 
already mentioned @-spodumene. 


IV. Hiddenite from Alexander County, North Carolina, U.S.A. 

Long, needle-shaped, pale green crystals, and emerald-green crystal- 
fragments, which are transparent and dichroitic. The specific gravity 
of this mineral at 25°,1 C. was found to be: dy=3,295 + 0,002 ; 
the refractive indices were: n, = 1,664 and n, = 1,674. The data 
for the specific density, given in literature, vary between 3,152 and 
3,189. Of a hiddenite from Alevander City, with specitic weight 


of: dy= 3,177, the analysis gave the following results : 
SUON 2. 63595.9/5 Pe Oraey lelve of. 
Al,O, : 26,58 °/, Na,O: 1,54 °/, 
iO G82), CaO: no trace. 


The sum of the principal constituents is here 97,35 °/,; the hue 
of the erystals is caused by the admixture of /eQ, which is oxydized 
in melting to Fv,O0,, giving a brownish-black or chocolate-brown 
colour to the solidified mass. Another hiddenite of the same locality, 
but of a paler colour, had: 64,35°/, SiO,, 28,10°/, A/,O,, and 7,05°/, 
Li,9, — consequently together: 99,5 °/, ; moreover: 0,25°/, LeO 
and only about 0,38°/, Na,O. The differences of the meltingpoints 
of these two kinds of hiddenite, were about 1° C. or less. In a 
series of observations, made with thermoelement IV, the melting- 
point was fonnd at 14565 M.V. + 410M. V.; after correction, this 
corresponds to 1418? + 41°C. , x.Th.). On cooling down the moiten 
mass, first an undercooling is observed to about 1255°C., if the 
temperature-fall was about 4° pro minute; then the temperature 
rose to 1262°C. during the solidification of the mass, being 150° C. 
lower than the real equilibrium-temperature. 

Another time we found an _undercooling to 1208°C., then 
solidification at 1214°C., — this being 204°C. lower than the true 
meltingpoint! Although this point of solidification is lower than that 
for the pure kunzites, it can have no essential signification whatever, 
being wholly dependent on the speed of cooling and other accidental 
circumstances. 


V. Spodumene of Somerd, Finland. 

A white, opaque eryptoerystalline and very hard mass. It was 
finely ground, and investigated in a manner, quite analogous to that for- 
merly described. The specific gravity at 25°,1 C. was : dy = 2,997 + 
0.050; the refractive indices were about : 2, = 1,658 and n, = 1,669. 
With the thermoelement /J’ the meltingpoint was found at 14649 
M.V. +5 M.V.; being, after correction, 1425° C. on the gasthermo- 
meter. Because of the inhomogeneity of the material, the meltingpoint 
is here not so sharply localized on the heatingeurves, as in the 
cases of the kunzites; on cooling the molten mass, solidification 
oeeurs in the neighbourhood of 1298° C. 

The substance solidified and heated for some hours below its 
meltingpoint, had a specific gravity at 25°,1 C. of: do = 2,398 ; the 
refractive indices were about: 1,510 and 1,518 for sodiumlight, 

just a little smaller than commonly with the -spodumene. The 
substance always shows very complicated aggregations of feebly 
extinguishing scales with undulatory extinction. 

If the original substance is not melted, but only heated during a 
longer time below its meltingpoint, the erystals are converted into 
the aggregations of the B-spodumene ; the specific gravity at 25°,1 C. 
was now: dy— 2,412 and the refractive indices about: 1,519. 


VI. Spodumene from Maine, U.S.A.; perhaps from Windhain. 
This mineral consists of long, opaque, prismatic crystals, looking 


Fig. 13. 
Dense #Spodumene of Someré, Finland. (X Nicols). 


259 


like porcelain, with predominant cleavage. The carefully selected 
material was finely pulverized, and investigated as described before. 
The specific gravity at 25°41 C. was: d= 3,154 + 0,002; the 


refractive indices were about: 7, = 1,656 and n, = 1,672. A micro- 
photograph of it between crossed nicols is reproduced in the fig. 13. 

The meltingpoint was determined several times with the thermo- 
element ///; the following results were obtained : 14669 + 13 M.V., 
being after correction: 1427° + 1° C. on the gasthermometer. Also 
in this case the meltingpoint is not quite so sharp as with the kun- 
zites, just because of the chemical inhomogeneity of the material. 

The obtained product had a specifie gravity : dyo = 2,336 at 25°,4 C.; 
the weakly birefringent, irregularly extinguishing scales, had refractive 
indices of about: 1,517 and 1,520; the birefringence is not greater 
than: 0,008. 

In fig. 8 a microphotograph between crossed nicols is given of 
the dense a-spodumene of Jaine; in fig. 9 the same preparation, 
molten and solidified into the 3-form is reproduced in the same way. 

’ The strong analogy witb the image of fig. 4, representing an arti- 
ficial 3-spodumene, made from L7AlO, and LiQ,, is obvious. 

Another preparation was not melted, but only kept at a constant 
temperature of about 1200°C. for some hours. The original «@-form 
appeared to be totally converted into B-spodumene ; the volume of 
the mass had increased then in such a degree, that the platinum- 


Fig. 9. 
Dense z-Spodumene of Maine, between crossed 6-Spodumene obtained by melting and crystallization 
Nicols. of the z-modification (X Nicols). 


260 


erucible was wrecked during the process. The substance showed the 
typical granular strneture of the crystal converted into p-spodumene 
with undulatory extinction and a mean refractive index of: 1,518. 
Phe specific weight at 25°,7 C. was determined to be : dy = 2,309, 
and. tobe 2oi7, at ood: 


§ 18. In all these experiments it was observed by us, that the 
platinumerueibles, in which the silicate was melted and solidified, 
showed a strong deformation, which increased every time that the 
experiment was repeated. As fig. 10 shows very clearly, this observed 
deformation is of such a kind, that it always appears as a dilatation, 
as if the silicate, like water, solidifies under a volume-expansion. 
The values obtained for the specific volumes of the erystals 
and of the g/ass, seem however to make this explanation rather 
improbable. We have tried by a series of systematic experiments to 
find out, ahen really this increase of the volume sets in, by measuring 
the diameter of the crucibles, after their contents had been subjected 
to different manipulations. In this way, we found, that by far the 
largest deformation of the crucibles took place, at the transformation 
of «, into 3-spodumene, which is accompanied by a volume-increase 
of about 30°),. When the substance is then melted once more, and again 
solidified, the deformation already present will be increased by the 


thermal expansion of the mass, and because the liquid substance is 


|o\3.b4 


1|\2 
Fig. 10. 


Deformation of the platinum crucibles after melting and solidification 
of the natural Spodumene. 
0. Origmal form of the platinum-crucibles. 


1. Pale yellow spodumene of Minas Geraés, Brasil. 
2. Kunzite of Sahatany-valley, Madagascar. 

3. Dense Spodumene of Someré, Finnland. 

4. Kunzite of Rincon, California. 


Ww 


61 


enormously viscous, enclosed air-bubbles are hardly squeezed out, 
but will rather expand in the mass itself, while the surface of the 
liquid can change its height only with extreme slowness. In repeating 
snecessively the melting and solidifying of the substance a number of 
times, the deformation-effect will be gradually increased to such an extent 
that, as fig. 10, N°.2 shows clearly, at last the crucible bursts. The 
gradual lowering of the liquid surface in successive experimeuts 
can be seen in those crucibles; in such a manner it often happens, 
that with a strong deformation of the platinum vessels, when they 
finally look like inflated balloons, the junction of the thermoelement 
emerges at last out of the surface of the liquid mass, so that the heat- 
effects on the heating-curves get gradually worse and will finally 
disappear totally. 


§ 14. To control the found meltingpoints, we have made a series 
of experiments to determine it once more (with the kunzite of 
Madagascar) by means of the quenching-method, which is to be de- 
scribed afterwards in connection with our experiments for fixing the 
temperature of beginning transformation. The quenching-system was 
first calibrated by means of meltingpoint-determinations, made by 
this statical method with lithiummetasilicate (1201°) and: diopside 
(139L°); the corrections to be applied to the measured temperatures 
appeared however to be practically zero. 

We found in successive experiments : 


Kunzite, heated during half an hour atl4600 M.V.and quenched in mercury: All crystallized 


7 P » Fe PAO ENS 5 Pee ee eAlleolasce 

” ” 2 Hp py LEOO MWS. 4 Js JN lbs: 

” ” ” Be unr AONE ~ Sa aor alleclasss 

” ” n Sut ay nee GSO en. ‘ ee i Glassand 
crystals. 

, . , PTE OOUIMEN Gear, F » »  ? Allerystallized 

” > > m3 wae 14690 M.V. ) > > ” : All glass. 


Thus, the meltingpoint was found to be 1428° C. (G. Th.), quite 
in accordance with the direct meltingpointdeterminations after the 
dynamical method. In these experiments we once obtained a product 
after longer heating on 14600 M.V., — just somewhat below the melting- 
point, — consisting of somewhat larger individuals. They appeared to 
be large, homogeneously extinguishing plates, whose birefringence 
was about 0,007, and with refractive indices of 1,518 and 1,519, 
like those of the 8-spodumene, obtained from artificial spodumene after 
melting and cooling. In convergent polarized light the same inter- 
ference-image as in the former case, was observed ; there can thus 

18 

Proceedings Royal Acad. Amsterdam. Vol. X VIL 


262 


hardly be any doubt, that the spodumene-modification, which is 
deposited from the liquid mass, is quite the same as that, which is 
discerned by us as 3-spodumene. There are no reasons to adopt the 
existence of a third modification, which on cooling should be con- 
verted into the 3-form, as occasionally has been done. 


§ 15. Before describing our experiments with this compound with 
respect to the study of the transformations into the solid state, the 
determined values are once more recapitulated in the following table. 

From this table (next page) we can see, that in general the melting- 
temperatures of the natural kunzites are considerably higher than those 
for the synthetical products, and further we can, generally speaking, 
deduce, that the meltingpoint of the kunzites are decreasing at the same 
time with the increase of specific gravity. (The specific gravities of the two 
first mentioned kunzites differ too little to give any certain argument 
for this view). Of the two kinds of dense spodumenes however, the 
mineral of higher specific density seems to have the higher melting- 
point also, although in this case the meltingpoints are too close 
together, and are moreover not sufficiently sharp, to give any certain 
argument for an eventual rational relation between the two mentioned 


constants. 


§ 16. Now we will proceed to the question, in what relation 
the different modifications of the compound LiALSi,O0, stand with 
respect to each other. That there are several of these modifications, 
can already be deduced from the mere fact, that the product o7 
solidification of the natural spodumenes is quite different from the 
original substances. 

Our investigations moreover have taught us, that there are really 
only to modifications, which can be discerned as a- and @-spodumene. 
Of these two forms the @-modification is undoubtedly the one to be 
considered as the more stable form at temperatures in the immediate 
vicinity of the meltingpoint. The question, however, then rises im- 
mediately: in what relation are «- and #-spodumene to each other? 
Are they enantiotropic forms, like e.g. wollastonite and pseudo-wollasto- 
nite? Or are they monotropic modifications, as e.g. they are observed 
in some forms of the pentamorphic magnesiummetasilieate ? 

After numerous experiments in this direction, we have come to 
the opinion that both forms of spodumene must be considered as 
monotropic ones with respect to each other, and a-spodumene, i.e. all 
kunzites, hiddenites, spodumenes of nature, must be metastable phases 
of the compound with respect to the B-form at all temperatures below 


263 


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264 


1400° C. Therefore it is neither possible to indicate an “inversion- 
temperature’, below which the e-form, and above which the @-form 
would represent the more stable phase: at all temperatures below 
its meltingpoint, the @-spodumene is the only stable form of the 
compound LZ7AlS7,0,. Under what conditions the «-form was always 
eenerated in nature, while it was till now never obtained in the 
laboratory from “dry” molten mixtures, may preliminarily be put 
aside. 

The reason however, that the «-modification, once produced, has 
remained so, notwithstanding its metastability with respect to the 
3-form, is to be ascribed to the enormous slowness, with which the 
transformation «— @ takes place. 


§ 17. To give an idea of this phenomenon, we will describe here 

a series of experiments, made with the purpose to answer the 
question, at what lowest temperature the transformation @a— @- 
form again will ocenr with a velocity just observable? Preliminary ') 
experiments had taught us that a long and little prominent heat-effect 
was. observed between 900 and 1000° C., if a larger quantity of 
finely powdered «-spodumene was gradually heated; and the micros- 
copical investigation also taught us soon, that within the mentioned 
temperature-interval, a transformation is going on with observable 
velocity. We therefore made the following series of experiments by 
means of the already mentioned statical method. For it is evident, 
that just with reactions proceeding so enormously slowly, this method 
can be used with great suecess, because 7 permits us to keep the 
studied substances at a constant temperature during an arbitrarily 
long time; in this way one can be sure that the reaction is thus 
completely finished, while the sudden chilling of the preparation in 
cold mereury will fix the momentaneous state of it in a most 
effective way. 
- The following data were obtained by observations with the thermo- 
element 1V; because the thermoelement was not placed in the mass, 
lut beside it, the whole furnace-system needed to be especially 
calibrated for this series of experiments. 

The calibration of the used quenching-system was executed by 
means of meltingpoint-determinations after the statical method, with 
substances, whose meltingpoints in terms of the gasthermometer were 
!) Vide also : G. Tawmann, Krystallisieren und Schmelven, p, 114. Spodumene (d=3,17) 
was transformed gradually into a much less dense substance (d=2,94), by heating 
on a Bunysexbarner during ten hours. The new product was attacked much more 
rapidly by HF than the original cubstance. 


already accurately known before. Only in this way is it possible, 
to find out, what temperature really corresponds to that, indicated 
by the thermoelement placed in the furnace. For this purpose we 
have made use of the meltingpoints of two compounds: L7,Si0, and 
MBoO,; the Li,ScO, melts at a temperature of 11956 M.V. on 
our standard-elements, the second at a temperature, corresponding 
to an E.M.F. of 7822 M.V.'). In this way we observed: 


| T 
| LinSiO3. | LiBO>. 


| | | 
Heating during along | | ‘ Heating during a long J : : 
_ time at a temperature, — State of the chilled time at a temperature, | State of the chilled 
_ at which the E.M.F. of system : at which the E.M.F. of | system: 
| element IV was: | element IV was: 
12060 M. V. All glass. | 7800 M. V. All glass. 
120205, All glass. TmOOwn All crystals. 
11980, All glass. | sors, Many crystals; a 
| | little glass. 
11940, | Much glass, afew crystals | 
TO 5, | All crystals. 
11930, All crystals | 
\| UTE 9 All glass. 
11950 sy, All glass. } 
Thus, when the furnace-element indicates 11940 | The meltingpoint of the LiBO, is thus reached, 


| M.V., the meltingpoint of Zz-.SzO3 is reached;the || if the furnace-element indicates 7780 M.V.; there- 
_ correction of the indicated temperatures at 1201°C. | fore the correction at 845° C. is: +42 MV. 

_ to reduce them the nitrogenthermometer, is there- | 

fore + 16M.V. 


From both these data for 845°C. and for 1201° C., the correction 
for every intermediate temperature is found by intrapolation; for a 
temperature of e.g. 965° C., it is + 28 M. V.; ete. It is with this 
number, that the just mentioned temperature (in M. V.) needs to be 
augmented, to be reduced to the nitrogengasthermometer-scale. 

Having in this manner determined the temperature-correetions for 
the whole quenching-system within the range of temperature from 
845° to 1201° C., we have chosen as an object for these experiments 

1) With the thermoelement IV three series of experiments were made, with 
heating-rates of 30, 40 and 60 M.V. per half minute. lor the lithium-metaborate 
we found thus successively as mean values: 7786, 7778 and 7781 M.V., — which 
gives as probable value: 7782 +4 M.V. The correction of element IV was + 40 
M.Y. at this temperature; the true meltingpoint thus being at 7822 M.V. = 845 C, 


(G. Th,). 


266 


the kunzite of Madagascar, and we tried to find in the described 
way the lowest temperature, at which a just discernible transform- 
ation of «¢— 3-form yet occurred. The reader may be put in mind, 
that the experiments 1—14 were made with a thermoelement, 
provided with a very thin protecting tube; in the experiment 14—20, 
this protecting tube was omitted, which appeared however to make 
no appreciable difference. 


| 


Indication of ther-| & | es Z \ 
moelement IV at) Ga | Soe 
No. | theconstanttem-|.EE | Des | Result of the Chilling: 
perature of healing Sf | 2S on 
| =I a= (=) 
(See ee wee Les 
| 6510 M. V. | 723° | 2 hours | Only «-modif.; no transformation. 
2 6800, 750 oy = idem 
Sm S80 S05 a Oe idem 
| | 
4 8450, COLA ee a idem 
ae | 9570, 1000 2 , | All s-spodumene. 
6 | O500/ eu wie mousenieoian idem 
7 9070 , | 957 CA No transformation; z-modification. 
8 9220 ,, 970 he idem 
9 9360 982 3 x ‘Partially transform.; «-, and #-form. 
| 
10 70s s 966 _ Probably the same. 
| | 
11 9280 , | 9715 Saar Partially 3-spodumene. 
12 9280 ,, 975 ey = All ?-spodumene. 
yt} 9260 ,, 913 | 4", Probably partially 3-form. 
| 14 9260, O73 .aeiSua All 8-spodumene. 
| | | 
Tis) 9260 , | 973 | 855 | All s-spodumene. 
16 |B) 9225 , 9170 | 8 , For the greater part: 3-form. 
Ya | | 
17 |2& \o160 965 | 4 , | All «spodumene. 
ae | | 
18 =e | 9200 ‘ 968 4 , Evidently partially g-form. 
19 |S8foi70 965.5 | 4 , | Some -modification, many crystals 
eae | of «-spodumene. 
20 9150, 964 | Was | No #-form; the transformation has 
| | not yet begun. 
| | | 
| | | 


In this case therefore an evident transformation has already taken 
place at 9170 M. V. (uncorr.), or at 9198 M. V. = 968°C. (G. Th.), 


267 


Similar experiments with the kunzite of Rimcon taught us, that this 
lemperature is situated somewhat higher, at about 995° C.; in all 
these cases however, only very long continued heating can lead toa 
complete transformation of the «-, into the 3-form. It is therefore 
quite evident, that at ordinary temperatures, and even at 400° or 
500° C., the transformation-velocity of «-, into @-form must be 
practically equal to zero; thus the « and 3-spodumenes can be in 
immediate contact with each other, during an undetermined long 
time, without transformation taking place. 

The transition of «-, into @-form is accompanied by an enormous 
increase of specific volume: it is augmented from 0.81 to 0.41, 
being about 33°/, of the original value. It often occurred that the 
heated and transformed powder had risen over the borders of the 
platinum crucibles. In the described quenching-experiments, the trans- 
formation could often be stated already, when the used platinum folium 
had not yet been opened: it seemed to be inflated by the increase 
of volume of the enclosed preparation. Microscopically it is observed 
that the larger crystals of the «-form, in this transformation primarily 
get innumerable cracks and fissures; afterwards they change into 
opaque, no longer normally extinguishing aggregations of fine, felty, 
or even broader needles, whose extinction is @/most normally orientated 
on their longer direction; they ean be recognized by their weak 
birefringence, as well as by their low mean refractive index : 1,519. 
The microphotographs fig. 7 and 9 may give some impression of 
the aspect of the two modifications between crossed nicols. 


§ 18. It may be expected, that the mentioned transformation- 
velocity will possibly be affected by some catalysers or by some 
fluxes in such a way, that it will show a discernible value already 
at considerably lower temperatures. 

Indeed we succeeded in proving, that on heating spodumene-glass 
with molten sodiumtungstate’) at temperatures between 850° and 
920° C., after 32 hours a partial crystallization has begun, which 
however was complete only after 65 hours of heating. The ecrystal- 
mass had a refractive index of 1,523, and appeared to be no other 
thing than B-spodumene; the determined specific weight was at 25° C.: 
yo a Devise 

1) The great difference between the specific gravities of the silicate and the 
molten tungstate, makes it necessary to use a platinum stirrer, to bring the silicate 
from the surface into the molten mass again and again. This stirrer was moved 
by means of a suitable electromotor-driven mechanism. 


268 


We then made similar experiments with @-spodumene (of Mann) 
in a mixture of 20°/, J/oO, and 80°/, sodiummolybdate at tempe- 
ratures below 650° C.; on heating during 122 hours on temperatures 
between 595° and 605° C., we obtained birefrmgent aggregates of 
felty needles of the @-modification, with often rectangular borders. 
The refractive index was 1,527, and while the aggregates of needles 
did not extinguish in any position between crossed nicols, the rectan- 
gular needles often showed a normally orientated extinetion. As in - 
ihe former ease, the product had also a pale lilac hue. 

Then we made the same experiment with a-spodumene (of /tincon); 
it was heated during 88 hours in the same mixtures at 595° to 
GO5° C. The small pieces of the «-form had got opaque and were 
converted at their borders or totally into the @-modification; the 
refractive Index was 1,519. 

More experiments were made, which all taught us, that from 
molten magmas, cooled under manifold varied circumstances, never 
was another thing produced, than either spodumene-‘“glass’, or 
B-spodumene; however we did not succeed in getting the a-form 
from dry magmas even a single time. As devitrification of spodumene- 
glass appears also never to give another phase than @-spodumene, 
— we are of opinion, that it may be considered as sufficiently 
proved, that the @-modification is the only stable modification below 
the melting point. The spodumenes of nature therefore certainly 
cannot be produced from dry magmas; they represent metastable 
forms of the compound, which are very probably generated from 
circulating solutions, that is by so-called “hydrothermal” synthesis; 
the natural forms of the compound only appear to be preserved 
by the enormously retarding factors, which prohibited the transfor- 
mation into the more stable €-form. Experiments are going on, with 
a purpose to produce the «-modification of the silicate by such 
hydrothermal synthesis. The results of these experiments will be 
discussed in a following paper. 


§ 19. Finally we can here give some data, concerning the lithi- 
wmnaluminate: LiAlO,. This compound was prepared by heating in 
platinum crucibles the weighed, finely ground and well mixed com- 
ponents, — lithiumecarbonate being taken instead of L7,0, — in 
our resistance furnaces once at 900° C., then at 1200° C. After the 
resulting mass had been pulverized, the heating was repeated and 
these manipulations repeated four times. Analysis of the beautifully 
crystallized, homogeneous mass gave the following numbers; 


269 


Observed : Calculated : 

Al, O7: 76,8 °/, TOL Uae fe 

LEOr: 23,2 °/, 23,0 °/, 22,7 °/, 

100,0 
Although a small excess of 47,0 was still present, the substance 
could be considered as -practically pure Z7A/O,, — the more so, 


as on heating, a certain amount of Z7,0 always volatilizes gradually. 
A preparation, heated only shortly at 1600° C. contained, as ana- 
lysis showed us, only 19,34°/, Li,O and 80,65 °/, Al,O,; no further 
change had occurred than that the crystals of the original prepa- 
ration had got inuch larger dimensions, while preserving their gene- 
ral properties. At 1625° ©. the substance shows no trace of melting, 
but decomposes partially, by the volatibility of the Z7,0. The pla- 
tinum is strongly attacked, 27,0, being formed, and thus the alumi- 
nate cannot be heated at higher temperatures, without changing its 
composition. The meltingpoint can thus be hardly determined; the 
substance must have been changed a long time before already into 
Al,O,, with perhaps a slight admixture of some lithitumoxide. Even 
in a “hollow thermoelement”, we were not able to melt the substance, 
notwithstanding it being heated up to 625° C. 

Microscopically the aluminate shows large, round-edged, hexagonal 
or octogonal plates (fig. 12), with a relatively high birefringence 


Fig. 12. 


Crystals of Lithiumaluminaie. (X Nicols). 


270 


and high interference-colours between crossed nicols. The refrac- 
tive indices were determined toe be: n, =1,604 + 0,001; n, = 
1,615 + 0,001 for sodiumlight; the birefringence was about: 0,012. 
No axial image could be observed. The specific gravity of the erys- 
tals at 25°,1 C. was: d,o = 2,554. 

In a following paper we hope to be able to give an account of 
the formation and the occurrence of the «-modification of the spo- 
dumene in nature, and to review the results so far obtained, also 
with respect to their geological significance. 

Laboratory for Inorganic Chemistry 
of the University. 

Groningen, May 1914. 


Physiology. — ‘On the survival of isolated mammalhan organs 
with automatic function.” By Dr. E. Laqunur. (Communicated 
by Prof. H. J. Hampurerr). 


(Communicated in the meeting of April 24, 1914). 


When studying the movements cf extirpated pieces of gut, I was 
struck by the following fact: a piece of gut which had contracted 
for 9 hours in a Tyrode-solution at 37°, to which oxygen had been 
added, and which had been left to itself at room-temperature, began 
to move again the next morning, after being heated and after a 
renewed addition of oxygen. However frequently such experiments 
with pieces of gut — in the way suggested by Magnus — have 
been carried out by various investigators, yet the possibility of 
keeping the gut alive for so long a period seems to be unknown. 
~ Further researches show, however, that the automatic movements 
of such pieces of gut are of much longer duration than one day 
and one night. The longest period, as yet observed by me, runs to 
more than 3 weeks. As many as 21 days after the death of the 
individual the movements of the piece of gut could be observed. 
This time probably exceeds everything hitherto observed in this 
respect on mammalian organs working automatically. 

We may compare with this, for instance, how long after the death 
of the individual the beart can be made to contract. The heart is 
indeed the only automatic organ, as far as | know, on which 
experiments have been carried out in this direction. KuLIABKo, for 
instance, discovered that when the heart of a rabbit, after being 
kept for 44 hours after death in an ice-chest, was perfused with 
Lockn’s solution, contractions again manifested themselves. The heart 


274 


sometimes beat for several hours at a stretch; certain parts of the 
heart are even said to beat on the 3, the 5, and the 7" day 
after death. It is a well-known fact that, when at the obduction 
air can penetrate into the cavity of the chest, this may give rise to 
spontaneous contractions of the right atrium — the w/timm moriens 
Halleri ov vather Galent. Vunrran states that he has observed these 
contractions in the dog for 93'/, hours after death. Rovussnau main- 
tains that he has seen these movements in an executed woman, 
29 hours after death. 

The human heart has also been made to contract independently 
after death. These attempts have never succeeded with adults when 
the individuals had been dead for more than 11 hours. (H. E. Herina). 

This could be done with the heart of a child 20 hours after death 
and in the case of a monkey as many as 53 hours after death. 
(KuntaBko, H&rtNa). ') 

Recently Carret and INnGrsrictsEN have stated that some tissues 
ean be kept alive for a long time after the death of the individual ; 
the tissues could even become differentiated under these circumstances. 
These experiments, however, have been taken partly with very 
small pieces of hardly differentiated tissues: this applies for instance 
to the muscle-cells of the embryonic chicken heart, contracting 104 
days after the death of the animal. (Carrer). And partly they relate 
to parts of organs (bone and skin) where it is not so easy to 
determine whether the cells are living still. To ascertain this the 
“surviving” tissues must be transplanted on another animal. It must 
be taken into account, however, that these tissues may have 
permanently lost their independence. Only with the assistance of the 
normal tissues of the animal on which they were transplanted, they 
had regained life. 

With regard to the following experiments on the movements of 
isolated intestines, the investigations of MaGnus have shown. that 
automatic movements are only met with, when besides the musele- 
cell the nervous system of Awerbach’s plexus has retained its activity. 
The phenomenon is, therefore, of a complex nature. 

Intestines can be kept alive longer than usual (++ 12 hours) only 
when the periods of activity are alternated with long periods of rest. 
This can easily be done, as we know, by lowering the temperature. 
At body-temperature the isolated gut works itself, sit venia verbo, 
to death, within from 10 to 14 hours, 


1) See the Summaries by O. Langenporr in Ergebnisse der Physiologie 1903 
and 1900. 


272 


For various reasons the intestines of smaller animals, mouse, cavia, 
rabbit, were chiefly experimented upon. The method followed here 
keeps the intestines longer alive in proportion as they are thinner. 
In reality this method is a very primitive one. In the intestinal wall 
there is no longer any circulation and the metabolism is therefore 
restricted to the diffusion through the whole thickness of the wall. 
Hitherto I have not succeeded in keeping the gut alive in ftyrode- 
solution, a medium particularly fitted for intestine-experiments, for 
a longer period than 5 days. Pieces of intestine which no longer 
moved in the solution in which they had been placed immediately 
after the extirpation, began to move again when the solution was 
refreshed. This can easily be explained. 

The experiments carried out by collaborators of Magnus, WEINLAND 
and Nwuxirch have taught that when the intestine is placed in a liquid 
medium, substances are formed which stimulate the intestine. That an 
accumulation of these stimulating substances, besides the usual decom- 
position products, and more especially besides the bacterial decom- 
position products, unavoidable in intestine-experiments,should impair 
the activity of the intestine in the long run ean easily be understood. 

If the temperature of the pieces is kept particularly low (+ 3°), 
then the intestine keeps alive much longer than if the temperature 
remains but litthe under the limit at which activity still manifests 
itself. Pieces of ecavia gut in tyrode-solution at 15° were already 
dead on the 38" or 4% day. 

If the temperature of the tyrode-solution was + 3°, the gut died 
only on the 5% day. 

To keep the gut alive for a longer period a medium is required 
resembling more than tyrode-solution the normal body-fluids. For 
this purpose I took Aorse-serum’*), the serum of the small animals 
experimented upon not being obtainable in sufficient quantities. 

Since oxygen must bubble through the fluid in which the gut 
has been placed, a great quantity of froth is formed if serum is 
taken instead of tyrode-solution. This can be avoided, however, by 
pouring a thin layer of olive-oil on the serum. It might be assumed 
as probable that serum would prove a better medium than a salt- 
solution on the strength of the many experiences obtained with the 
surviving heart. (Wurre, Howni., Greex, Wanpen, with hearts of 
warmblooded animals, Guririm and Pike with hearts of mammals. *) 


1) Horse-serum can be oblained by the method, described by HAMBURGER and 
often applied in his laboratory, | take this opportunity of again thanking my 
colleagues De Haan and Ouwewwen for the readiness with which they always 
provided me with horse serum, 


It is true, cases have been mentioned where a frog’s heart, which 
beat no longer in sheep serum and could no longer be stimulated 
mechanically, was made to contract again by Rtina@ur’s” solution 
(Waxprn). Yet the possibility is net excluded that in these cases the 
strange serum has gradually had a poisonous effect. Therefore I 
shall also leave it an open question if the time during which the 
eut keeps alive would not be longer still if, instead of horse-serum, 
serum of the same animal, if possible of the same individual, were 
used. 

The experiments of INGrBeiarseN with tissue-cultures in auto-, 
homo- and hetero-geneous sera have demonstrated the relative 
superiority of autogeneous serum to serum of other individuals of 
the same kind, and of these two sera to heterogeneous ones. INGr- 
BRIGTSEN has not used horse-serum; this seems to be a particularly 
indifferent medium. Numerous experiments have shown that this 
serum is a much better medium for the gut than tyrode-solution. 
The gut of a cavia, for instance, kept in tyrode-solution, was dead 
after 5 days; when kept in horse-serum another piece of the same 
gut still moved after 21 days. 

The experiments were carried out in the following manner. 


The animal, a cavia for instance, is killed by decapitation, 

+ 20 em. behind the stomach a piece of the small intestine, long + 40 c.m. 
is cut out and divided in Tyrode-solution into 8 pieces long 4—6 c.m., called 
a—h. 4 of these (a, b, e, f,) were placed in Tyrode-solution, 4 others (¢, d, g, /) 
in horse-serum. 

Oxygen is led through the 8 glasses. The pieces a, e, ¢, g, are connected with 
a writing apparatus lo a cymographion (method of Magnus) 

To ¢ and g olive-oil is added. The movements of these 4 pieces having been 
registered at + 37°, they are slowly cooled down. Then the current of oxygen 
is stopped. The glasses a, e, and the reserve-experiments b, f, remain at room- 
temperature (+ 15°), the glasses c, g and the reserve-experiments d, h are exposed 
lo a temperature of + 3°. The pieces a7};, eT, ¢T\, and g7T, remain connected 
with the writing-apparatus or are removed with it. 

On the third day after the death of the cavia the pieces a, e, c, and g are 
connected wilh the cymographion whilst oxygen is led through, and are slowly 
heated to 40°. All the pieces move, but not so much as the first time except 
Sz, the movements of which have become greater. The fluid in all 8 glasses is 
refreshed after being cooled down and saturated with oxyen as on the first day. 
On the sixth day all are heated ete. just as on the third day. Piece 77; moves 
no longer now, not even after the Tyrode solution has been refreshed. The reserve 
piece “7); does not move either: therefore in Tyrode solution at + 15° the gut 
dies before the 4th day The three other pieces ¢7, °S);, and 9Ss still move, 
the first two less again than last time. On the 6th day everything is heated again 
etc. Piece e7; moves no longer, not even after the Tyrode-solution has been 
refreshed. Nor does the reserye-piece /7'; move: hence in Tyrode-solution at + 3 


D174. 


the gut dies before ithe 6th day. Piece “S|; does not move either. On the other 
hand the reserve-piece 4S), is still in motion. Movements of 7Sg are still greater 
and have the same frequency as before. The three fluids are renewed etc. On the 
Sth day only “S; moves distinctly: hence in horse-serum at + 3° death before 
the 8th day 

On the 10, 13, 15, 17, 20, 22ud day 7S; moves distinctly, but the movements 
have become smaller. On the 25th day no movements. The reserve-piece 2S; got 
fresh serum for the last time on the 24nd day and is for the first time connected 
with the cymographion on the 27th day. It does not move; only its tension 
decreases when heated. Hence in horse-serum at 3° the intestine dies after the 
22nd and before the 25th day. 


Hunan gut can also be kept alive for a comparatively long 
time ‘). A piece of colon, obtained after an operation, moved still 
after 86 hours. And an appendix, kept in horse-serum, described 
no straight line on the cymographion after as many as 6 days. 
There were slight but distinet contractions, which ceased when the 
intestine was cooled down to 25°. Finally I may mention that a 
human vas deferens was still alive in tyrode-solution after 30 hours. 


Summary. 

Isolated pieces of mammalian gut can be kept alive during a long 
time, much longer than the periods found hitherto for other auto- 
matic mammalian organs. For this purpose the medium in which 
the gut has been placed must occasionally be refreshed whilst it 
is of great importance that the temperature of the solutions should be low. 

In Tyrode-solution of 15° the gut dies after 3 days, at 3° after 
+ 5 days, in horse-serum at 15° after + 7 days, at 3° after more 
than 21 days. 

Also pieces of human intestines still showed signs of life after 
they had lain for 6 days in horse-serum at + 14°. 


Groningen, April 1914. Physiological Laboratory. 
'!) I am indebted to Prof. Kocn for his kindness of providing me with pieces 
of human gut. 


975 


Physics. — ‘/sothermals of monatomic substances and their binary 
mintures. XVI. New determination of the vapour-pressures 
of solid argon down to — 205°’ Comm. N°. 140a from 


the Physical Laboratory at Leiden. By C. A. Crommenin. 
(Communicated by Prof. H. Kamernmen Ones). 


(Communicated in the meeting of March 28, 1914). 


The vapour-pressures of solid argon, which are communicated 
below, form an extension of and have partly to replace those published 
on a former occasion. ') 

The measurements were made in the usual vapour-pressure apparatus 
for low temperatures. *) 

The manometer on which the pressures were read was constructed 
after the model used by G. Hots for his measurements on ammonia 
and methyl-chloride to be published shortly: this form of manometer 
gives perfect security against leakage. 

The method of conducting the measurements gives no oceasion 
for special remarks: we refer the reader to the previous paper. It 
may be mentioned however, that the temperatures were measured 
with a gold-resistance thermometer, as below — 200° gold is preter- 
able to platinum. This thermometer was very carefully compared 
with the standard-platinum-thermometer Pty. 

I am indebted to Mr. P. G. Carn assistant in the physical Labo- 
ratory for the measurement and calculation of the temperatures and 
for the comparison of the two resistance-thermometers referred to. 

Table I contains the results of the observations and the deviations 
from the Rankru-Bose-formula : 


log Peoex. =arnB + bra T—! + erp T—-2 + dep T-3, 


with the following values for the coefficients 


agp + 6.6421 crg = — 0.677438 x 101 
bea = — 3.7181 10? dre = + 0.280384 « 108 


1) CG. A. Grommetin, Comm. Leiden. N°. 138¢c. The measurements were repeated 
because shortly after the publication doubt arose as to the accuracy of the determi- 
nations at the lowest temperatures (see note on p. 23 of Comm. N®. 138c). The new 
measurements showed this doubt to be justified, the observation at — 2069.04 
being found altogether wrong and the one at — 179°.62 not very accurate. The 
remaining observations of Comm. N® 188¢ correspond well to those published 
here. The probable cause of the errors must be air having leaked into the argon 
at the low pressures: but [ cannot explain how it is that this was not noticed 
during the measurements. 

*) H. KamertinaH Onnes and C. BraaK, Comm. N°. 107a. 


bo 
~f 
o> 


TABLE |. Vapour-pressures of solid argon. 


pat @ (Celsius | ia | Percentagerdeviations 
ig | Ne SN cae) TUT eee ee 
Ceyesee | | MCCAY: formula. | formula. | 
26 Nov. | XXIII ~189.64 | 0.6554 | 49.78 | +0.20 | +1.33 | 
| XX |” 191/31 | 0:5175. "|" 39.30 ot oa 

XXVI 195.60 | 0.2749 | 20.88 |  +0.35 Ss 

XXVII 197.25 | 0.2153 | 16.35 | 2.16 +0.15 

28 Nov. XXVIII 200.97 | 0.1113 8.456 | —0.94 |) ==o029 
XXIX | 202.21 | 0.08931 | 6.783 | —0.89 —1.49 

XXX | 203.78 0.06740. 5.119 | —0.04 +0.59 

XXXI 205.32 | 0.05043 | 3.830 | 10:36 [|p ="2:79 


and from Nernst’s formula (treated simply as an empirical formula) 


A 


log Peoex. = 7 Se SUR es Ding Ps <G) 
with the coefficients 

A= — 907.49 G — -+f- 20.851 

B= + 0.010899 D = — 6.9057. 


The values of the coefficients in both formulae hold for p in ems. 
mercury. 

The comparison with the formula which Sackur has deduced 
from Nernst’s heat-theorem 


a en pene (oft a 
( SS = SS UG — SSS = a0) = 
pe ewan wa 23k) T 23R 


is given in table II. 

For details as to the manner in which the various values have 
been calculated the reader is referred to the previous paper. It will 
be seen that the agreement is satisfactory at the higher temperatures 
while at the lower temperatures the deviations become very large. 

Finally 1 have caleulated the heat of sublimation of solid argon 
from the simplified CLapryron-Crausivs-formula 


RT? (dp 
Aso .Vvap. = — == ° 
P dT CO"X., 


| TABLE II. 

| ue A 

Pee pW) p(R) 
—189.64 | 0.655 0.618 

191.31 0.518 0.507 

| 195.60 0.275 0.286 | 
197.25 0.215 0.226 | 
200.97 | 0.111 Onin 
202.21 | 0.089 0.124 

| 203.78 | 0.067 0.107 
205.32 | 0.050 0.094 


Calculating (Ge from the above Rankrve-Bosz-formula the 
c coex. 

following values are found for the heat of sublimation expressed in 

calories per gramme of substance at the various observation 

temperatures 


TABLE III. 


Calculated heat of 
| sublimation of argon. 


In coneluding [ am glad to express my hearty thanks to Professor 
H. Kamertincu Onnus for his continued interest in my work. 
19 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


278 


Physics. “Further experiments with liquid helium. J. The ime- 
tation of an Amekre molecular current or a permanent magnet 
hy means of a supra-conductor. (Cont.). By Prof. H. KAMERLINGH 
Onnes. Communication N°. 140¢ from the Physical Labora- 
tory at Leiden. 


(Communicated in the meeting of May 30, 1914). 


§ 5. The main experiment repeated. Although the original experi- 
ments on the persistence of a current which is started in a closed 
supra-conductor have established the fact that the diminution of the 
current with the time is very small (at least if it is assumed that 
in the phenomena hitherto unknown magnetic properties do not play 
an important part), still for the magnitude of the change only an 
upper limit could be fixed. As no change of the current was obser- 
ved, this upper limit was determined by the uncertainty in the 
measurement of the current. The only fact established so far was 
that, if the change had been greater than 10°/,, it would have 
been observed. 

In repeating the experiment it was attempted to determine the 
change itself or otherwise to reduce its upper limit, in so far 
as the conditions under which the experiment had to be made 
allowed this. The same supra-conducting lead-coil was used. As before 
the current was produced in the closed conductor by induction in 
order that the circuit might be kept free from connections other 
than of lead fused together‘). The current was again measured by 
compensating the action of the coil on a compass-needle by means 
of a current in a subsidiary coil. The arrangement was however 
improved by this coil (of insulated copper wire) being placed in a 
small vessel with liquid air in a fixed position with respect to the 
needle. When the compensation was obtained, the experimental coil 
was turned 180° about a vertical axis and again compensated with 
the current in the second coil reversed, the magnetic moment of 
the experimental coil being deduced from the mean of the two 
observations. 

If the diminution of the current can actually be calculated 
from the residual micro-resistance given in Comm. No. 138, viz. 
10.8 K. ; 

———_=—0)5) <10—®, oriawith Topo K. 134 2’): riog x, = 37, the time 
19060 Kx. 

1) An attempt is at present being made to manufacture a supra-conducting 
current-key. 

2) This value given already in Comm. N® 1406 is a more accurate value than 
the one given in Comm. N°. 153. 


of relaxation, with 1 = 10%, would come to about 270000 seconds 
ovr 75 hours. In that case the current would fall by 4°/, in three 
hours. It was hoped that it would be possible with the improved 
arrangement to establish a diminution of that amount. 

The experiment was made with a field of 189 gauss at a tempe- 
rature of 1.°7 K. The current amounted to about 0.4 amp. (as 
before no account was taken of the possibility of magnetisation or 
of induced circulating currents inside the supraconducting material) 
and during about 2'/, hours no diminution of the current was 
observed; it was then necessary to admit a fresh supply of helium 
into the cryostat: during this operation the temperature rose tem- 
porarily to 4.925 K. During the next hour the current was found 
to undergo a gradual diminution and to approach asymptotically a 
new value of about 0.56 amp. which did not show any further 
change for 1°/, hours. The observations during the two periods 
mentioned render it probable, that the change does not attain the 
value of 4°/, in 3 hours as calculated above. 

It was considered possible, that the changes of shape of the 
helium-liquefier and the cryostat during the process of condensation 
and transfer of the liquid helium, as well as a possible change of 
zero of the compass-needle which after the magnet has been removed 
is still near various iron parts of the apparatus, might have had an 
influence on the values of the current as measured at different 
moments. Judging by the correspondence of the various readings 
the accuracy was smaller than had been expected. In again repeat- 
ing the experiment therefore two compensating coils were used by 
which compensations on the east and on the west could be effected. 
They were mounted each in a small vessel with liquid air on a 
fork-shaped stand and could be rotated about vertical axes in such 
a.manner that the distance of the axes could not change. The same 
needle served for the compensation on both sides. Guiding pins 
guaranteed the same position cach time of the needle relatively to 
the compensating coil which was being used. The common support 
of the two coils was moveable parallel to itself in a horizontal 
direction on a slide and by means of marks it was possible to place 
it each time in the same divection and the same position relatively 
to the vertical axis of the experimental coil. The axes of the three 
coils were provided with horizontal divided circles moving along 
fixed pointers. Each measurement consisted of 8 readings in the 
obvious combinations of 4 positions both with compensation on the 


left and on the right. 
In the experiment with this improved method of reading care was 
19* 


280 


also taken, that the current did not rise above the value at which 
no further change had been observed at 4°.25 K. The current was 
therefore raised to only 0.22 amp. (approximate value calculated 
as before from the observed magnetic moment of the coil), so that 
the supply of a fresh quantity of helium would probably not have 
the disturbing effect which had been noticed in the previous expe- 
riment. The temperature used was 2° K. In the beginning again a 
fall of current was noticed which must however be considered as 
uncertain, inter alia owing to the possibility of the changes of shape 
of the apparatus and the change of zero of the needle not having 
been sufficiently eliminated yet in these observations. In the three 
hours subsequent to the initial period no further diminution was 
observed, the last observation even giving a small increase. Still in 
this experiment the accuracy could not be considered greater than 
about 2°/, of the measured moment and, as it was found impossible 
to continue the experiment, beyond three hours, again only an upper 
limit for the change could be established, to be put at about */, °/, 
for current and induced magnetisation combined. Taking all the expe- 
riments together it may be considered as probable, that the change 
of the current is less than 1°/, per hour which raises the time of 
relaxation to above 4 days. 


§ 6. Upper limit of the residual micro-resistance according to these 
experiments. So far no contradiction has arisen in reasoning on the 
assumption of the existence of a residual micro-resistance whieh 
below the threshold-value’ of the current again obeys Onm’s law. 
On this view the upper limit of this micro-resistance for lead, which 
in Comm. N°. 188 was placed at 0,5 10—!° of the ordinary resi- 
stance at 0’, can now on the basis of the above observations be 
moved further back to about 0.3 10~!" or 0.2 10—!" of the resistance 
at the ordinary temperature. 


§ 7. Some of the control-experiments repeated. In the previous 
paper a few other experiments beside the main experiment were 
described : some of these have now also been repeated. 

Again we did not sueceed in conducting the experiment in which 
the windings are placed parallel to the field, the coil cooled below 
the vanishing-point while in the field and then the field removed 
in such a manner, that the compass-needle, when brought near the 
cryostat after removal of the electro-magnet, did not show any 
deflection. After the action of a field of 400 gauss at 4°.25 K. a 
current of O.1 amp. was found in the coil. This would give 0.045 


281 
amp. with a field of 189 gauss, the same as used with the other 
experiments, whereas the main experiment at the same temperature 
and inducing field had given 0.4 amp. 

More satisfactory was the experiment in which first a current is 
produced in the coil — analogous to the currents in resistance-free 
paths as imagined by Weser for the explanation of diamagnetism — 
and then destroyed by the removal of the field: an almost complete 
compensation was obtained in this case. The experiment was made 
with a field of 189 gauss. This result is of special importance as if 
practically disposes of the supposition mentioned in the previous 
paper as possible, although very improbable, that magnetic properties 
of the material of the coil might play an important part in the 
phenomena. 

The current in the coil changes with any new magnetic field 
applied and with any further change in it, or with any change of 
position relatively to the field. In this respect the influence of the 
earth-field may be noted. The current in the coil, when placed with 
its windings at right angles to the meridian, will assume a slightly 
smaller value in the one position North-South and a somewhat larger 
value in the opposite position Sout-North than in the position East- 
West, which is practically the position in which the experiments 
were made. In our experiments this action was however too small 
to be taken into account considering the accuracy which could be 
attained at the most. 

It may be observed that our conductor carrying its current in the 
absence of an electromotive force, when undergoing the relatively 
small action of the field of the earth, is analogous to the AMPERE 
molecular currents (in the form of circulating electrons) which play 
a part in LanGrvin’s theory of magnetism, when they experience a 
diamagnetic action on being brought into a field, in accordance with 
Lorentz’s theory of the Zrrman-effect. 


§ 8. The experiments repeated with the circuit open. 

So far it has been constantly assumed, that the magnetic properties 
of the material of the coil play but a secondary part in the pheno- 
mena observed, when the experiments were arranged so as to 
produce a permanent current. This view was based firstly on the 
difference in the results with the windings parallel and perpendicular 
to the field during the cooling in the field and secondly on the 
compensation found on applying and removing the fiela after the 
conductor had already been cooled to helium-temperature. Further- 
more that the part of the effect which is independent of the circu- 


289 


a 


lnting current must be ascribed to the lead itself, was to be inferred 
from the fact, that the current is quenched, as soon as the tempe- 
rature of the coil rises somewhat above the boiling point of helinm 
and passes the point which, as being the vanishing point for lead, 
has a special physical meaning for this substance. 

In order to obtain further information as to the part of the 
phenomenon which depends upon the material itself, the experiments 
were repeated after the lead-wire connecting the ends of the coil 
had been cut, so that the circuit was no longer closed (apart from 
possible short-cirecuits in the coil). 

This time the experiments with the exception of one could only 
be performed at 4.°25 K: still there does not seem to be any objection 
to applying the results for the explanation of the irregularities which 
had been left unexplained in the main experiments, although these 
had been mostly carried out at a lower temperature. 

In all the experiments a certain residual effect remained, which 
was reduced to about one tenth when the windings were parallel 
instead of at right angles to the field and in the latter case was 
fairly well independent of the field. The amount of this effect cor- 
responded to a moment which was equivalent to a current of 0,05 
or 0,06 amp. in the closed circuit. In one of the experiments, the 
only one in which the temperature was lower than 4.°25 K., viz. 
about 3° K., the moment was estimated to be equivalent to as 
much as 0.07 amp. The effect with the circuit open is thus very 
much smaller than in the main experiments. The share born in the 
effect by the frame of the coil and the lead independently of closing 
the circuit may therefore be put at less than '/, of the total effect 
in the main experiment. 

As a check on former experiments the following additional expe- 
riments were made with the coil with the lead wire cut. 

In the first place at the ordinary temperature after joining up to 
a ballistic galvanometer the induction was measured arising from 
putting on or taking off the field with the windings in the position 
in which they were supposed in the previous experiments to be 
parallel to the field. The induction was found to be '/,, of the effect 
in the position at right angles to the field. This observation may 
contribute to the explanation of the residual effect observed in the 
experiments in helium in the position with the windings parallel to 
the field. 

In the second place a known current was sent through the coil 
and its strength measured by the same method as used in determining 
the moment of the experimental coil in the experiments with the 


Z 283 


lead cireuit closed. Although the matter requires further elucidation, 
it would seem to follow from this measurement, that a few of the 
layers of the coil are short-circuited. After opening the cireuit a 
residual moment remained in the coil as before which was destroyed 
on raising the temperature slightly above that of the helium-bath. 


Physics. — “Further experiments with liquid helium. K. Appearance 
of beginning paramagnetic saturation.” By Prof. H. Kamertincu 
Onnes. Communication N°. 140d from the Physical Laboratory 
at Leyden. 


(Communicated in the meeting of May 30, 1914). 


The question, whether paramagnetic substances would show a 
saturation-effect at high field-strengths, has always been considered 
a very important one. Although it could hardly be assumed, that 
the susceptibility would remain independent of the field at higher 
strengths than were attainable, still so far at the highest fields 
available if appeared to be the case. Lanervin’s theory brought 
the explanation, why so far all attempts to find paramagnetic satu- 
ration-effects had remained unsuecessful. According to this theory 
the magnetisation appears to be determined by the expression 


a= ——, where 6, is the magnetic moment of the molecules per 


eramme-molecule, A the gas-constant, 7’ the absolute temperature 
and #H the field. As long as a remains below 0,75, the changes of 
the susceptibility with the field escape the ordinary method of obser- 
vation and at the ordinary temperature even a substance as strongly 
paramagnetic as oxygen gives for @ with a field of 100000 not more 
than about 0,05. As I pointed out at the 2°¢ International Congress 
of Refrigeration at Vienna (1910) this theory shows that lowering 
the temperature is the means by which the observation of para- 
magnetic saturation might be attaimed and that helium-temperatures 
are the most suitable for the purpose. In fact as the absolute tem- 
peratures to which one may descend by means of helium are 70 
and even 150 times lower than the normal temperature, the result 
will be equivalent to raising the magnetic field at which the obser- 
vation is made 70 or 150 fold. 

I have lately at last been able *) to fulfil my desire to attack by 


1) Viz. by the acquisition a short time ago of an electromagnet (built according 
to Weiss’s principle and utilising his friendly advice) the interferrum of which 
leaves sufficient room at fields of 20000 for experiments with liquid helium, 


284 


this method the problem of paramagnetic saturation which is also 
fundamental to Wriss’s theory of ferromagnetism. In the first place 
it was necessary to have a substance which might be expected to 
obey Curt’s law, which also follows from Lanervey’s theory, down 
to helium-temperatures ; in the second place the substance must have 
a high value of 6,. Botb properties I hoped to find combined in 
crystallized gadolinium-sulphate, a quantity of which Professor URBaIN 
some time ago had very kindly put at my disposal. 

Earlier investigations in conjunction with Purrter and Oostrrauis had 
shown, that gadolinium-sulphate follows Curte’s law down to the free- 
zing point of hydrogen and does not show any sign of saturation, which 
as LanGEvin’s theory shows, if it existed at that temperature, would 
be ferromagnetic in its nature, as paramagnetic saturation at the 
value of a which could be reached would not yet be clearly obser- 
vable. The number of magnetons calculated according to Weiss is 
large (38). That gadolinium-sulphate would still obey Curm’s law at 
helium-temperatures I felt justified to infer from the fact, that it is 
a “diluted” paramagnetic substance. The gadolinium-atoms, separated 
as they are e.g. by the water of crystallisation, are at great distances 
from each other, and this Dr. Oosrrrauis and I in Comm. N°. 139e 
found a favourable cireumstance to Curim’s law being valid down to 
very low temperatures. 

The experiments have given a confirmation of LanGevin’s theory 
which is at least qualitatively even now complete. Before an opinion 
can be formed as to the quantitative agreement various corrections 
will first have to be investigated. The most important of these which 
must not be neglected, especially when the validity of Curte’'s law 
is to be tested, is the demagnetising action of the paramagnetisation 
itself, as the latter attains exceptionally high values. As an instance 
I may mention that with 0,345 gram of gadolinium-sulphate at 2° K. 
in a field of 15 kilogauss there was observed an attraction amounting 
to over 100 grammes. Another circumstance that une should keep 
in mind is that the object of observation consists of small crystals 
packed on each other. 

The measurements consisted in determining the attraction in a 
non-homogeneous field, the gadolinium-sulphate in the eryostat being 
cooled first in liquid hydrogen under normal pressure, next in hydrogen 
under reduced pressure, next in helium boiling at ordinary pressure 
and finally in helium under 4 mms, the apparatus and the fields 
being the same each time. 

The measurements at the boiling point of hydrogen (20.°3 K.) 
had the object to obtain the force at a given point for a given 


285 


strength of field for controlling the values derived from ballistic 
calibrations. I hope to return to the details of the measurements 
and the arrangement of the apparatus afterwards, when an accurate 
quantitative comparison of the results with Lancevin’s theory will 
have been made. It is as yet impossible to decide, in how far 
deviations are present which might be attributed to the existence 
of a small zero-point energy which would manifest itself in the 
manner in which the saturation changes, as well as in a deviation 
from Curtn’s law at weak fields. It seems, however, that these devia- 
tions are not sufficiently large to disturb the general aspect. 

On this oceasion I wish to confine myself to communicating the 
general aspect of the results as laid down in the adjoining graphie 
representation on which the experimental numbers may also be read 
with sufficient accuracy. The curves represent the observed attractive 
force as a function of the square of the field on the axis between 
the poles. This field was read as a funetion of the current from a 
calibration curve. 


2 


&. 

Curve I refers to 20.3 K, curve Il to 14,°7 K, Il to 4.°25 K. and 

IV to 1.°9 K. Each division along the horizontal axis corresponds to 

about 90 kilogauss, along the vertical axis to 25 grammes. The ratio 

of the force to the square of the field on the axis of the poles per 

unit of susceptibility was about ',, neglecting small changes in the 
topography of the field. 


286 


If the susceptibility does not depend on the field and its topo- 
graphy remains the same, the curves are straight lines. The small 
deviations from the straight line at 20.°3 K are probably chiefly due 
to errors in the topography of the field, seeing that according to 
earlier more accurate determinations we had to await within the 
limits of the experiments a susceptibility independent of the field and 
therefore in this graph a straight line. By means of the deviations 
from the straight line at 20.°3 K the curves for the other tempera- 
tures have been provisionally corrected. It will be seen that for a 
given field these curves are the more strongly curved the lower the 
temperature to which one descends, in accordance with LANGEvin’s 
theory. Within the limits of accuracy to be expected in connection 
with the neglect of the various corrections referred to above the 
tangents of the angles of elevation of the tangents to the curves at 
the origin appear to be inversely proportional to the temperature as 
required by Curie’s law and the deviations of the curves from the 
tangents as expressed by the ratio between the ordinates of both 
for a given abscissa are strikingly similar to the deviations of 
LANGEVIN’s curve for the magnetisation as a function of the field 
expressed in the same manner. The nature of paramagnetic magne- 
tisation is very clearly revealed in these measurements at helium- 
temperatures. 


Mathematics. — “On some integral equations.” By W. Kapreryn. 


1. In a memoir “Recherches sur les fonctions cylindriques” (Mem. 
Soe. Roy. Se. Liege dime Série t. VI 1905) we gave the solution 
of the integral equation 


(2) = J 918) Lei ds Perce so 3 (i) 
0 


in this form 


a) ae 
Q(z) = ae La fro —— — CP Meomo. 6 3 4) 


where the functions /;, represent Beenie functions of order &. 
This solution rests upon the relation 
, 


: Ela 1G BOC) fib 1 Bic Bo. 
{Zo = aoe HGS a ) i es 


xf n 
0 


from which the following theorem may be deduced. 


If 
F(z) = ¢,1 («) + ¢,£,(e) + ¢f,(@)+--.- »- + + (4) 
then 
P a 3) ; : 
fr (2) er SE es eed) ane eG) 
0 te 
The object of the present paper is to show that more general 
integral equations may be solved in the same manner. 


De Tet 


am 
. 


Fe) = | vA) (eA. a 2 6) 
6 
where p represents an integer, and let 
F(®) = Cptilp4i(#) + ¢pelp+o(%) + .--- 
(3) = 6,2,(8) + 6,4,(8) + 6,2,(3) 4 --- 


then 
- 
S Oe) = ss by, Jue I, (@—8) dp. = - . = (7) 
p+ 10) e 


0 o 
Therefore the integral equation (6) will be solved if we can 
determine the coefficients 4 in function of the coefficients c. 
We shall first show that 


u =| I,()L,(«—p)adg 


can be expressed in a series of Bessei’s functions. 
By differentiating we get 


d . U,(e—P 
Sel yr (7) at (@—P) ap 
da. da 


raf I, (8) — NS) ag 


d3 3? 
Now 
2 ia = 2 
aC) Ces) iy Fy se Se 
da® «—p dx ( )B? 
or 
ad? I,(a« —p) p 1 dl(«—Pp) 
} ( / 
= (a6 (e—6)— — - 
da? st Epa D) (w—p)? p28) p da 


288 


where the second member may be reduced by means of the relations 
P 


aan L, (ew—B) = 3 [Lp41 (@—B) + Ips (e—B8)] 
d 
re I, (c—6)=4 [Zp—1 (e—p) — Ip4i («—)]. 
Therefore 
int 3) (= 1 1,1 (w —8) pti, 1 («—B) 
eas I, (e—8) =- ! = pana!) 
div a a—p 2 z—Pp 
and 
du p-l (4. 1p-1(e-8) Bet Ty41 (e—8) 
: =— —— | /7,(¢e — dp + — 3) ——__— _ dp 
pare oer elf eee 
0 0 


or, according to (3) 


dt } i L{l n+p—1 (w) 4e Ln4p4i (a ‘)] 


au p) te (w) Ds 


This differential equation holds also if eer 
Now the general integral of this equation 


u=Asine + Boose + (n+p) fon aah). ate ®) as 


gives the required value of w, a the constants A and B are 
determined by the conditions 


du 
z= 0 i ==) ——*() 
dx 
du 
A=) u = 0 = == Il (== 709 = 1) 
da 


Thus we obtain generally 


4 = (n+p) fis (av 8) = ae 8) a 


and when n= p=0 
SINK 
Introducing now the known expansions 
sin (e«—B) = 2 [J, (e —B) — I, (e«—8) }|- J, (e—B) — ...] 
and 
sin & = 2 (I, (x) — J, (x) + J, (2) «. | 


we have according to (3) 


289 


== Leer (2) — Ln4p+s (#) + Intpts («) — seo) 
thus in all cases 
x 
Tk (3) Ly («—6) dg = 2 [Zn t (x) — L,4p+3 (2) ap dl ntp-ts ( az (5) 
0 
Applying this result, the equation (7) takes the form 
2) enim (w) i by [Lntp+t (2) aaah Ent p43 (x) =e cod] 
p+ n=0 
and comparing the two members we have 
Cp+1 — 2b, 
Cp+2 —— 26, 


CS ta 26, + 26, 
Cp-+4 = 26, oo 2b, 
ete. 
thus 
ip a hee eae sacl ee 
OSes 2 PS 2 Di Chae 9 7 25. 5 z 
and 
2 bi F ep --3 ; ae 4 
gx (3)= ig) sae £(8)+ wana ED fe (gaan Eee (ay. (Q} 


The solution of ih integral equation (1) in the form (2) may be 
easily deduced from this equation. For putting p= 0, we obtain 


1O=2 0+ Ot ros 


In this case 


SF (#) =e, +, (@) + 6, LZ, (x) + ¢s 7, (%) + --- 


oS 


I, (2) +. 


thus 
df Cy C3 C4 ©, 
== Sh) +240) +2 10+ 5740+... 
and 
df 
@p («) — — =e, J, (2) + ¢, J, (&) + 
dau 


which, according to (5) may be written 


I («—p 
vont (10 Po. 


3. We shall next show that the solution (9) may be written in 
the same manner as the solution (2). It is however convenient to 


examine first the special cases p= 1, 2, 3. 


290 


I. — | 
Let @)= | ¢ (8) 1, (a — B) dp 
‘0 
then 


f) (#) = 2 g (2) =| ¢p (8) [8 Z, (e —- 8)-— 1, (x — B)] dB. 
0 


Multiplying these equations respectively by 1 and 4 


and adding 
we find 


fey 


2? f%) (w) + 4 f (0) = 2p (e) 4 fv (8) [1, (@—@) + 4, (@—8)] ap 


0 
 esriGeee 
= 2p (#) + 7 y (3) pus ip 
10) 
thus 
. I («—B 
2 (@) — [2/9 (ON — 4 LF = — 4 f 9)” ap. 
1) 


Now, according to (5 
> 5D 


xr 


i I («—p 
2| p (@) = Pas = byl, - Od, se bef, ee 
e WOK 


0 


or, with the values of 6 from (9) 


=tlel, +¢4+¢%+-- 1] 
+ $[e.7, tet, +¢,2%, + --] 


which by means of (5) may be written 


Therefore the solution may be put in this form 


2g(w) — [2° fFE(@)| — 3 [fo] = — ofan Me me dp . (10) 


yo ee 
Differentiating 


291 


P= (v (8) Z, (e—8) a 


we obtain 


2f(2) =r (8) (1,—1,] 48 


29H 200 + fi (8){— 47, + 312,—J,] dp. 


Thus 


av 


ak a? TA. eee 
227 Me)+ 2AM Bele) — [HOLL +L MP=24 (0) —8 (6G) 


e & 
0 0 


where 


1 - 1 
=> flew = ec. eal, es... <i] 


1 
see Les l + ¢f, + ¢,I3 +...] 


— 3) I,(2«—B) 
= |e) —e at > sf fe) dB 
0 0 
This gives the solution 
me =v se I (ie 
24 (0) — [24f)(2)] —4[2/M(a)] =f jG)" aa fi (0) ap 
—p z—Pp 
U U 


i pc. 
By differentiating 


J(#) = Jv (B) Z, (eB) dB 


we obtain 


247° (a) = {o(B) 21, + 1.) a8 


292 


27 (o) = 2 (0) + f(B)L— 51, + OL —A1, + La 
0 
Multiplying these equations respectively by 4, 5, 1 and adding 
we get ‘ 


[247 (@)J 4- 5[ 2277 (@)] + 4[ A(2)] = : v)| wi fu ee 
ue 8 
= 2y (x) + 12f) (8) a = dg 
0 
where 
if tle 8) 
6 fv) gy BL, EOL, + OT + 
e vU—t 
0 
== i(C, I. sp os Sp Oar ao) 
SF $ (cl, = cL, == ORI + -.-) 
ae a I (#—p) 4 7 , L(e7—B8),, 
= » {78 per dp + 2. WO ane 
0 0) 


In this case therefore the solution takes the form 


2y (a) — [24a] — 5 BVO) — 4 el = 
48 oe fre Pa, (12) 


4. Proceeding now to the general case, we may expect, A;{”) being 
constants, 
ly (w)-A,' P ) Paes AC )(x)} =A i Pp) [2P—1f pt \(x)] -A, (p)[2P—3 fP = 3)(x)} = 
Bs 
= (—1)?. 4p [vi 3) 


0 


I2,(«@—8) 
ee . (18) 


If p be even the last term in the first member is — AY [27 (w)], 


2 


and if p be odd it is ~ Able v)]. 


The second member now reduces to 
> (z—B 
2pfutey™ vie ae = b, 1 Ta, bate ela ee 


0 


293 


= $ [pile, + p4olo,pi + cp43lopte + . | 
+} [ep4itopte+e42lopt3t+¢,43lots + ---] 


thus 
zr z 

on (nc. t2(@—B) 1p P—! (re — p+l Ty 4i(a- 

2p fate) a PP (ray ae Baas EA gyi = V3 (14) 
0 0 


Substituting this value in the equation (13) we see that g(x) may 
be expressed in differential coefficients of the function J(2) and two 
integrals. To determine the law of the coefficients A,(”), A,”, A\™, 
A,)... we put together the values for p=1, 2,...10 in the 
following table: 


p AO SAC VAG) | 2A) A VA) AG) 
1 1 3 

2 \ 4 

a 1 5 4 

4 1 6 8 

5 1 7 13 4 

6 1 8 19 iz 

7 1 9 26 25 4 

8 1 10 34 44 16 

9 1 11 43 70 41 4 
10 1 12 53 104 85 20 


Examining this table we see that 
A,(P) = A\P-Y + AS p—®) 
A,r) = As ps) of A ip 2) 


A,(p) = A,(r—1) 4+ A,fp—2) 
(p even) 
OD) —— y—1) (p—2) __ (p— 2) 
AY, — is + Ape =4+ A 
(p odd) 
(p) =. 
Ay = 4 


If therefore the coefficients of order p— 2 and p —1 are known 
those of order p may be found. To verify the results we may 
remark that if 

TAM=S, 
we must find 
Sp = Sp—2 aia Sp—1 . 
The resulting values of these coefficients are as follows 
20 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


294 


AK (p12 ed.22) 
A?) ==/)) + 2 — 1a -) 


1 
A= > (p?+p—4) (p=3.4.5...) 


rare Bye 
Ae) 31 (p—4) (p?+-p—6) (p=5.6.7...) . (15) 


eS 


1 PORK 5 
A fp) = ai (p—5) (p—6) (p?+p—8) (p=7.8.9...) 


1 
er (p—68) (p—T) (p—8) (p?+-p—10) (p=9.10.11..) | 


where the law of succession is evident. With these values the equa- 
tions (13) and (14) give the required solution. 


4. To generalise the preceding results we will proceed to examine 
the more general integral equation. 


f(a) =[9(@)K(@—A)dB . . . . . . (16) 
J 


assuming that the functions f(z) and A(x) may be expanded in series 
_ of Brssex’s functions 
Se) = ¢,1,(@) + el .(w) + e,2,(@) + «. 
K(«) = a,l,(e) + a, f,(e) + a,1,(a) +... 
which is the case if these functions are finite and continuous 
from O to 2. 
If now 
—p (x) = b,L,(x) + b,1,(x) + 6,7,(x) + ... 
the second member reduces to 


x 
S355) yl. I, (8) L) (e—8) a8 = 
U 

2S ayy pyle) — Lp-+943 1b Iptags — +] 
Thus, comparing the two members, we find 
= 10- 
» = 2a,b,+2a,), 
c, = 2 (a,—a,) b, 4+ 2a,b, + 24,6, 
c, = 2 (a,—a,) b, +2 (a,—a,) 6, + 2a,b,-+4 2a,, 
etc. 


Cat 


c 


which give 


‘ 1 
26, = —e, 
ay 
ob ee a, C, | 
2b, = —_, 
Dx Ce Os) 
1 4 Oc! 
26,=>— 4, a, ¢, 
ay 
g,—4, a, ¢, 
a, 0 C; 
1 fa a 0c 
1 0 
2b, =— ; 
a,’ |a,—a, a, i, Cs 
a,—a@, 4,—a, @, ¢, 
ete: 


Therefore g(v) may be written in this form 


ay 0 0 0 
a, 00 
] a, 0 1 1 a, a, 00 
24(«)= —e,?1,+ == (aie ee Cp hy OT ipee 
a, Gea anic. a, Gy \a,-a, a, a, 9 
a,-a, &, Cy 
@,-@; @—a) a, ¢, 
‘ a, 0 00 
a, 0 0 
1 Gace 1 1 a, ay 0 0. 
“tee ott gal PANEL Ul i It. 
a, |a, V| a, a |a,-a, a, a, Cy 
a,-a,a, 0 
a,-@, a,-a, a, 0 
ay 0 0 0 
a 0 c, | 
iT 1 \4, a, ONG: 
= 0,/,+— iD 
a 311 GON ae 7 sche. 
a," a a,-a, a, a,0 
\a,-a, a, 0) 


@,-4, a,-a, a, 0 


0 1 
1 a; ae, ADD) 

+ > z J,+-. 
0 |a,—a, a, a, 0 


a, 4, a,-a, a, 0 


or 
20% 


296 


1 
2¢(«) = lan (1,42, | c,l,+ “M :) 


0 
We 
0 (c,2,+¢,2,+-¢,2,+ a) 
ke, 
1 
+s make a, 0| (¢,f,-+-¢,2,+¢,1 4.4 - -) 
: a,—a, a, 9 
\d, 0 0 1 
pie. Ol | 
+ ar | (c,I,+¢,1,+¢1,+--) 
a, |a,-a,a, a,9 
a,-a, a@,-a, a, 0} 
+ ete. 
If now 
f(e)=eJ, + Cale aie Cas ci 
we have 


df 
pa am Sead ie SS Gye 


da 
= (c,1, 33 ty, =e o,f, a as -) 


thus, according to (5) 


c.J,tel, +¢/, +... = 0th frosts ap 


and by the same formula 


In—\(e@— 8) dp 


e,In + ¢Inpi + eslng2 + ++ = 0) {7 259 
0 


Introducing these values we have 


ee a ee ae 


where 
a. Oru 
eal Ea 1 | | 
anaes fee ala! 0| A, a,? Ci a, 0 | ie (17) 
|@,—Ay A, 0 | 


Remarking that 
nIn(a« —B) 
«—Bp 


this result we may write 


= $ [Znsl@—8) + Ing (eB) 


497 
2¢(2) = = 2 a aes Ane ae $ J@l—A AGS BAC er dg ar 
0 


: | (18) 
ASME rAnane—oa| 
0 


When the integral equation 


2D («) = | W(8) K (« —8) dp 
0 


is given, we find by (18) 
eo = A, /,(«) + A,4(e) + 4,4,(2) + -- 


Therefore = = (A,+-A,42)4, pov) be expressed in function of wp. 


For 


LETTS a hey WI oma eo Pea fae aa) 
and, differentiating again 


ee a -B) 
A,I,(a) | AD, +A TD, +-.=4 = +29+-A,F,—A,7,—2 | w8)— a 
av a — Bp 


0 
thus 


x 


2 Ged mal Ij(e—f) _, 
(Ay 4 Appa) = 475 + Bh + A, AL —2 | WG) 7 a3 
: . assy 


e 
0 


5. We now proceed to give some applications of formula (18). 
First let the integral equauien be 


a=fu (3) I, (e—8) dB 


then 
Gy SS ly Gh = 0 So SW) 
hence 
A =I ARO AL ale A =A! 10) 
thus 
x 
9 9 df % ) 5) 
2p (e) = 2 + 4 (F(8) (22, (@—B) + 22, @—B)] 4B 
0 


or 


998 


= 

oli" f+ fan se 
—p 
which agrees with (2). 
Considering the integral equation 
z 
Ho) = [x (3) 1, ayaa 
0 


the formula (18) is not applicable because a, — 0. In this case and 
assuming a, =— 0, we have 


1 
2p) (@) = ae (Ql ORIEN 55) 


Ie as 
— Notre vom ae ee) 
a, aa 
; a Oma 
tall 4s Gen0> (0,0 geri) 


where 


PY Di ce Ie er i 


oe . T, («—f) 
oy Be =e ~ = Gi 
tah $n = 2S r ff @) ee 
0 
I, esl, 4 pals 2 2) as 
c | oe == 4 —— + 27 — 2 f 7 (8B) ——_ c 
TO Sik dx? “oe fi Bp t 


. af —8) 
2p (x) = B, se : afi (8) ee pe 


aah 
+ B, 17 (8) 1 fe—8) 13 
w—B 
0 


299 
or 


—é) 


af i ‘ (@ 
+(2B,+B,)/—2 rf) oe a+ 


2g (7)=4B, an? +2B, Ie 
) 


a A RB 
+f me [(\B,4+B,)1,(e—p)+2B,1,+3B,1,+. Jade. 
0 
Now putting 


we have 
Bell Bi) 13). == 1 Bi == == eat 0 
thus 
xr 
: Gap >  fj.«—B 
24(«)=4 de ok 2 K(8)- <> d3 


e 
( 


which agrees with (10). 
Finally let the integral equation to be solved be 


x 


¢(@) cos (e—B) dg 
In this case 


thus 
i — Av —=0 , Ano 7 A= 0h, ALS Aes er eel peel 


and, according to (18) 


ie 
24 (2) = 2 ay ence @)+ 80,4 87,4 °8/,+...] de 
0 
which, by means of the known relation 


Pia DT (aya Tey ee SS 


may be written 


or 


300) 


Geodesy. —- “Comparison of te measuring bar used in the base- 
measurement at Stroe with the Dutch Metre No. 27”. By H. G. 
vy. p. Sanpe Baknuyzen, N. Winpesorr and J, W. Dinewrink. 


In the summer of 1918, the Government-Commission for Triangu- 
lation and Jevelling measured a base of about 4320 metres, under 
the direction of Prof. H. J. Hruvenmk, on the high road between 
Apeldoorn and Amersfoort, near the Railway-station Stroe. 

The measurements were made with the base-apparatus of the 
“Service géographique de Varmée” at Paris, which was lent through 
the courteous help of the Director of that service to the Government 
Commission by the French Government. 

The measuring bar of this apparatus is an H-shaped invar-bar_ of 
four metres length, provided with two very sharp end lines at the 
extremities, between whieh three intermediate lines are drawn, which 
divide the measuring bar into four parts, a, 6, ¢ and d, each one 
metre long. : 

Previous to the base measurement here, this measuring-bar had 
been compared several times with the métre international at Breteuil ; 
these comparisons had shown, that the length had undergone some 
slow changes, as is often the case with invar-bars; it was therefore 
important to determine the length shortly before and after the base- 
measurement. 

In April 1913 therefore a comparison was made at Breteuil, but 
as the comparator there had to undergo some repairs, the comparison 
could not be repeated in the autumn of 1918; it was therefore 
decided to compare the measuring bar in this country with one of 
the two Dateh platinum-iridium metres, viz. with No. 27, by means 
of the comparator which had been supplied by messrs. RepsoLp and 
Sons in 1867 with the base-apparatus for the triangulation in the 
East Indies, and which is now mounted in the geodetic buildings in Delft. 

From the experience gained in previous measurements we did not 
consider that sufficient accuracy could be obtained with this compa- 
rator, especially on account of the inferior quality of the microscopes ; 
on this account it was decided to order two new micrometer-miecros- 
copes from Zeiss (in Jena) which were delivered in the autumn of 
1913, so that in December the comparator was ready for the comparison. 

We are very much indebted to Prof. Hruveninx, who arranged 
everything for the measurements and placed a room in the geodetie 
buildings, and an instrument-maker at our disposal for some weeks ; 
and further to the ‘Commission for the preservation of the stan- 
dards”, who allowed us the use of metre 27. 


301 


il Arrangement of the comparator. 

A complete description of the comparator can be found in Dr. J. 
A. C. Ouprmans, “Die Triangulation von Java, erste Abteiling”’ ; we 
may therefore confine ourselves here to a short account of the 
arrangement. 

A wooden case over four metres long inside, contains a long iron 
carrier, which can be moved upon rails from one side of the ease to the 
other, at right angles to the length. Upon this carrier the measuring 
bar and the metre with which it is to be compared, are placed 
parallel to each other, while the metre with the box in which it 
is placed can be moved along the carrier in the direction of its 
length, and can so in turn be placed opposite to each of the four 
parts a, 6, c, and d of the measuring rod. 

The wooden case is further provided with a strong iron frame 
to which the micrometer-microscopes are attached at a distance of 
exactly a metre and which can be moved upon rails, independently 
of the carrier, above the measuring bar and the metre. 

The first thing to do is to place the metre opposite the first part 
of the measuring bar, parallel to and at the same height as the 
bar, and to push the carrier upon which they both le as far as 
possible sideways across the case, until it touches a pair of correc- 
tion screws. If everything is properly arranged, the microscope 
frame upon its rails can then be placed so, that the two microscopes 
are just above the end lines of the metre, or the part a of the 
measuring bar. If the carrier is then moved to the other side of 
the case, where it similarly touches two screws, the microscopes 
will be directed just above the end lines of part a or of the metre. 

By focussing with the micrometers accurately upon the end lines 
of the metre and of part @ in both these positions, it is easy to 
find the difference in length between them, expressed in micro- 
meter-divisions. By subsequently placing the metre successively opposite 
to the portions 4, c, and ¢ of the measuring bar, and making the 
same observations, the data are procured, by which the length of 
the measuring bar can he determined in metres. : 

In order to be certain that in the successive measurements of 
portions a, 6, c, and d the microscopes were each time directed 
upon the same points of the division lines, small brass plates 
provided with a point in the middle were fixed on the middle of the 
bar near the division lines, in this way fixing a line along the middle 
of the measuring bar. The correction screws at the sides of the case, 
(against which the carrier moves up in ils sideways movements) 
were so adjusted, that these points came exactly under the fixed 


802 


horizontal wires in the two microscopes. As care was taken, that 
the moveable micrometer wires were parallel to the division lines, an 
influence of a small deviation of the point upon which the micros- 
copes are directed need not be feared. 


2. Microscopes. At our request the microscopes were so con- 
structed, that on the obiective-side the course of the rays is tele- 
centric; they have a 30-fold magnification, and the illumination of 
the division lines is not sideways but central, by means of a prism 
with total reflection, which is placed behind the objective in the 
tube of the microscope, and occupies half of the field. The light 
from a small electric lamp falls through an opening in the tube of 
the microscope upon the dull face of the prism, is then reflected by 
the prism vertically downwards through the objective, falls upon the 
reflecting surface of the metre or the measuring bar, and is thus 
reflected vertically back into the microscope. With an electric lamp 
of a few candles the illumination was excellent, and the division 
lines were seen as very fine black lines. 

3. Temperature. The exact determination of the temperatures of 
the metre and the measuring bar is a matter of great importance. 
In order to make the changes of temperature as small as possible 
we endeavoured, in the first place, to keep the temperature of the 
room as constant as possible. For this purpose the windows were 
covered with thick curtains, and the central heating was shut off. As 
only a small amount of heat was conveyed through the floor and 
walls, the temperature did not change much, and only rose a little 
from the presence of the observers, and the burning of a few gas lamps. 

All the metal parts of the comparator were shut off from the 
outside air by wood and other badly conducting material, outside 
which only the eye-pieces of the microscopes protruded ; the measur- 
ing bar was moreover entirely enclosed in a thick aluminium case 
and the metre in a brass box, in which there were only small 
openings for the reading of the division lines and the thermometers. 
The protection of the metre from the radiating heat was less effective 
than that of the measuring rod, so that in half of the measurements, 
during which the observer was on the side of the comparator nearest 
to the metre, it was found advisable to cover the outside wall of 
the comparator with a layer of badly conducting material, which 
gave a greater constancy of temperature. 

For the determination of the temperature of the metre and mea- 
suring bar, upon the horizontal faces on which the division lines are 
drawn a thermometer A was laid upon the metre, and on the measur- 


303 


ing bar two thermometers B and C, the last two about a metre from 
each extremity. Moreover there were placed in the comparator case 
a registering thermometer ), two thermometers // and F upon the 
outside of the aluminium case about above the thermometers B and C, 
and two thermometers G and #/ at the two extremities of the comparator, 
which were read through glass-covered openings in the end-walls. 

On the whole the temperature readings were of such a nature, 
that there is every reason to believe that the readings of the thermo- 
meters A, B and C may be taken as the temperatures of the metre 
and the measuring bar. 


4. Programme of the measurements. It was arranged, that the 
measurements should be made by the two engineers of the Govern- 
ment Commission for triangulation and levelling, A. Winprsorr and 
J. W. Dieprrink, and a member of the commission, H. G. v. p. SANDE 
Baknuyzen. Each of these made a complete series of measurements. 
Mr. Witprsorr and Mr. Dirprrink arranged everything beforehand, 
so that (1) metre and measuring bar were parallel to each other 
and at the same level, (2) the micrometer wires were parallel to the 
division lines and showed no parallax with regard to the division 
lines, (8) in the extreme positions of the carrier the division lines of 
the metre and of the measuring bar appeared in the correct position 
in the field of the microseopes. In the adjustment of the level of 
metre and bar, so that no parallax could be detected of the micro- 
meter-wires with respect to the division-lines, the adjustment of one 
of the observers was always checked by a second or third. 

When the carrier had been placed in one of the extreme positions 
and the microscopes were therefore directed upon the end lines, say 
of the metre, the observer placed the micrometerwires of the left- 
hand microscope twice in succession upon the line, then took four 
readings with the right-hand microscope. and finally two with the 
left-hand one. In the middle of these eight readings the thermo- 
meter on the metre was read. The carrier was now brought into 
the other extreme position, so that portion a of the measuring bar 
came under the microscope. In the same way as for the metre, 8 
readings were taken with the microscopes, and readings of the 
thermometers. The observer then returned to the metre, and in the 
same way took seven sets of observations in succession, alternately 
upon the metre and the selected portion of the measuring-bar, each 
consisting of 8 readings. 

A series of observations of this kind, which lasted about a quarter 
of an hour, we shall henceforth call an observation-series. 


304 


Hach of the three observers made two of these observation-series 
in succession. 

After these six series, the metre was turned round in its case, so 
that the mark which first showed on the left hand side now lay 
on the right hand side; and in the same way as at the beginning 
of the measurements, the position of the metre with regard to the 
measuring bar and the microscopes was then properly regulated. As 
the comparator case had to be opened for this, there was a disturb- 
ance in the equilibrium of the temperature. An hour or 1‘/, was 
therefore allowed to pass before fresh measurements were begun. 
As in the first position, each of the three observers then took two 
series of observations in this second position. 

For the determination of the temperature in the comparator, at - 
the beginning and at the end of the 6 series with the same position 
of the metre, the thermometers /, /’, G, and H were read. These 
readings served only to ascertain, whether disturbances of tempera- 
ture had oecurred in the comparator. In none of the series which were 
used for the determination of the length of the measuring bar was 
this the case; there was therefore no further use made of the 
readings of the thermometers 1, /, G, and H, any more than of 
the records of the registering thermometer. 

As in the computation of the results the differences of the readings 
of the right-hand and left-hand microscopes are used, the influence 
of a personal error of adjustment will disappear from the results, 
if both end lines, the micrometer wires and the optic images in the 
two microscopes are exactly alike. This complete equality however 
does not exist. The lines are, as far as can be seen, all equally fine 
and faultless, but the distance of the micrometer wires is smaller 
in the one microscope than in the other, so that the appearance of 
the line, when it is placed between the two micrometer wires, is 
different in the two microscopes. In order to eliminate the personal 
error arising from this, the observations would have to be repeated 
after exchanging the microscopes, or else with the microscopes in 
the same position, but the observer standing the second time on the 
other side of the comparator, so that the microscope which was first 
on his right hand, is now on his left. 

The latter method is simpler than the former, and had the further 
advantage (over the changing of the microscopes) that the observer, 
who first stood nearest to the measuring bar, is now nearest to the 
metre, and an irregular influence of the heat radiated by the observer 
will thus be also, at least partially, eliminated. 

On these grounds the observers, after they had compared each of 


305 


the 4 portions of the measuring bar with the metre, while standing 
on one side of the comparator, repeated the observations standing 
on the other side. 

To distinguish the observation-series from each other, we shall 
call those which were made while the observers were in their original 
position with respect to the comparator, A, those in which they were 
on the other side, £6, the series in which the mark on the metre 
lay to the right of the observer 7, that in which it was on the 
left 7, while the first of two identical series we shall call 1 and 
the second 2. For each portion of the measuring bar each observer 
therefore took 8 series of observations Ar,, Ar,, Al,, Al,, Br,, Br,, 
Bi,, Bl,. Care was taken, that when the first series was begun 
with the metre, the second identical series should begin with the 
measuring bar. 


5. Runs and errors of the micrometer screws. For the purpose 
of determining any possible changes in the runs of the micrometer 
serews, the length of the millimetre divided into 10 marked on the 
measuring bar near the end lines was measured every day before 
and after the measurements, with both of the microscopes. From 
the results it appeared, that the value of the run, which was approxi- 
mately 200 micromillimetres, did not change perceptibly. As, however, 
it was not certain, that the millimetres on the measuring bar were 
of exactly the correct length, the absolute value of the run was 
afterwards determined by measuring out a distance of 1 centimetre 
divided into millimetres on a measuring rod of nickel-steel belonging 
to the Observatory in Leiden, supplied by the Société Genevoise, 
the errors of division of which had been accurately determined in 
Breteuil. For all the measurements the same value of the run is 
assumed, viz. 198.69 micromillimetres for the microscope marked I 
and 199.82 micromillimetres for the unmarked microscope. 

Moreover the periodic errors of the micrometer screws were 
determined in the observatory at Leiden, by measuring distances 
equal to a half and a third of a turn. The continuous errors were 
determined by measuring a larger distance, with portions of the serew 
situated symmetrically with respect to the zero. 

For micrometer | the correction formula of the readings in parts of 
the divided head, was found to be: 0.18 Sim (wu + 17°); the influence 
of the term dependent on the double of the reading was imperceptible. 

In the unmarked microscope no periodic errors could be detected 
by the observations. 

The continuous errors were imperceptible in both microscopes. 


306 


6. Reduction of the observations and results obtained. The micro- 
meter readings are all reduced with the above mentioned values 
for the run of the screws in micromms and for the periodic errors 
in micrometer I. 

The errors of thermometer 4570 belonging to the Dutch platinum- 
iridium metres, which was used for the temperature-determinations 
of metre No. 27, were determined by comparison with two thermo- 
meters standardized at Breteuil, and by separate determinations of 
the freezing point. It appeared, that between 0° and 30° the ther- 
mometer is free from errors, except the error of the freezing point, 
which was —0.48°. The determinations were made by Mr. H. C. 
Vorkers, lecturer at the Technical University at Delft. 

For the thermometers 153855 and 15356 belonging to the invar- 
bar both the errors of division and the correction for the zero are 
negligible. 

In the reduction of the length of the metre and the measuring- 
bar the following coefticients of expansion were used. For the metre 
the value communicated by Bosscua in his paper: ‘Relation des 
expériences qui ont servi a la construction de deux métres étalons en 
platine iridié, comparés directement avec le metre des archives” and 
which from 0° to ¢° gives an expansion for the metre in micromms 
of: 

8.4327 ¢ + 0.00401 7’. 

For the measuring bar, the determination made at Breteuil was 

used, which gives for the expansion per metre in micromms; 
1,6245 ¢ + 0.001065 ¢?. 

After the introduction of these reductions, the three observers 
obtained the following results for the lengths of the 4 portions of 
the measuring-bar, each about a metre in length, diminished by the 
length of N°. 27 both at the temperature of zero. These results 
are the mean of the observations of one series. 


Portion O—1. 
WILDEBOER DIEPERINK BAKHUYZEN 


Position A Position B Position A Position B Position A Position B 


1, —29.70 —27.43 —26.65 —27.39 —27.93 — 26.40 
l, 28.25 27.84 28.28 27.19 28.60 27.13 
1, 29.25 28.39 28.85 27.94 29.89 27.96 


iP 29.01 28.95 28.89 28.23 29.49 27.91 


307 


Portion 1—2. 


WILDEBOER DinPERINK BAKHUYZEN 
Position A Position B Position A Position B Position A Position B 
i, —99.31 —95.46 —98.59 —96.73 —97.96 —96.10 
E 99.61 95.28 98.64 96.02 97,65 96.22 
iP 98.82 95.338 97.95 96.99 97.30 95.69 
ip 99.96 95.18 98.50 96.7 97.69 94.94 


Portion 2—8. 
WILDEBOER DIrPERINK BAKHUYZEN 
Position A Position 6 Position 4 Position B Position A Position B 
Poe ee —— 12200) 12.2570) 1.23.64 2352) 199-95 
i 22.25 122.22 122.26 123.00 12239 123.03 
r 122.72 AO ioe, 121.18 121.04 122.85 1:23:35 
7 122.00 121.46 120.75 122.24 121.96 122.83 


Portion 3—4. 
WILDEBOER DIEPERINK BAKHUYZEN 
Position A Position B Position A Position B Position A Position B 
1, —144.49 —14348 —143.28 —143.45 —144.09 —143.22 
i 144.55 143.58 143.96 143.37 143.938 143.28 
ry 144.91 144.00 144.09 143.69 145.10 144.57 
r 143.70 144.08 143.98 143.65 144.44 143.48 


In order to eliminate the effect of personal errors the means 
were now formed from the observation-series A and JB, those 
two series being combined in which the metre was in the same 
absolute position in space, not relatively to the observer, i.e. Al, 
with £r,, Al, with Sr,, Ar, with Bl, and Ar, with Bl,. In this 
manner the following results were obtained : 


WILDEBOER. 
Portion O—1 Portion 1—2 Portion 2—3 Portion 3—4 


—29.04 —97.32 —122.24 —144.20 
28.60 97.39 121.85 144.31 
28.34 97.14 122.36 144.19 
28.42 97.62 122.11 143.64 


Mean 28.60 97.37 122.14 144.08 


308 


DIEPERINK. 


Portion O0—1 Portion 1—2 Portion 2—3 Portion 3—4 


——Ora9 9) 1187 —143.48 

28.25 97.70 122.25 143.80 

28.12 97.34 122.41 143.77 

28.04 97.26 NSH 143.67 

Mean 28.18 97.52 122,10 143.68 
BakHUYZEN. 

Portion O—1 Portion 1—2 Portion 2—3 Portion 3—4 

—27.94 — 96.82 — 108} 144033 

28.25 96.29 122.61 143.70 

28.14 96.70 122.90 144.16 

28.29 97.45 122.49 143.86 

Mean 28.16 96.82 122.86 144.01 


If the sum is 


taken of 


the lengths of the 4 portions of the 


measuring-bar, we get for the length of the whole measuring bar at O°: 


Measuring bar = 4 x Metre 27—392.19 WILDEBOER 
4 So Metre2 (=a Oras DIEPERINK 


” 


55 = 4 xX Metre.27— 391285 
Mean for the three observers : 
Measuring bar = 4 « Metre 27—391’.84. 


BAKHUYZEN 


7. Mean errors. The errors in a series of observations are caused 
by the pointing- and reading errors of the microscopes, the change 
in the distance of the microscopes, erroneous determinations of 
temperature and personal errors of observation. 

Owing to the excellent optical qualities of the microscopes and 
the fine sharp end lines, the errors in the reading and pointing of 
the microscopes are small. From the observations for the determination 
of the periodic screw-errors we found for the mean reading-error, 
from the mean of two observers, + 04,32: this error leads to a 
mean error of + 0,17 in one series of observations. 

The influence of other sources of error are difficult to determine 
separately. We shall therefore try to calculate their combined effect, 
in different ways, in order to find out, what systematic errors are 
to be feared, and how the series of observations are to be combined 
in order to obtain a result in which the effect of the systematic 
errors will be as far as possible eliminated. 


309 


In the first place it was investigated, whether there was a systematic 
difference in the results of a series of observations according to 
whether the microscope was pointed 8 times on the metre and 
4 times on the measuring-bar, or 4 times on the metre and 3 times 
on the measuring-bar. For this purpose the mean was first formed 
of corresponding series in the positions A and #4, in which the 
number of times that the microscope was pointed on the metre and 
therefore also on the measuring bar, was the same. According to 


these averages the mean error of observation in micromms was: 


WILDEBOER DIgPERINK BAKHUYZUN Mean 
Ott 0.366 0.509 0.420 (I) 


After this the average was formed of corresponding series in 
A and & in which the aumber of times pointed on the metre and 
on the measuring bar was unequal; according to these averages the 
mean error of observation for a series was : 


WILDEBOER DinperiInk BAKHUYZEN Mean 
0.496 0.330 0.440 0.428 (IT) 


From the agreement of the two means we may infer that there 
is no systematic difference in the series with 3 or with 4 pointings 
on the metre or measuring bar. 

It was next investigated, if there was a systematic difference in 
the results of series in which the metre was in a different position 
relatively to the observer, i.e. in the results of the series / and 7. 

This was done in two ways. 

1. The differences were found of the corresponding series in 
Which the observer and the metre were in the same position in 
which differences the systematic error referred to plays no part. The 
mean error for a series 7 deduced from this is: 

WILDEBOER Divperink BAKHUYZEN Mean 
0.450 0.346 0.492 0.434 . (IIT) 

After this the mean was formed of all the corresponding values 
found with the same position of the observer, in position / as well 
as position 7 of the metre. 

The deviations of all these values from their mean, in which the 
influence of the systematic error is present give the following values 
for the mean error of a series. 


WILDEBOER DiePERINK BAKHUYZEN Mean 
0.454 0.594 0.636 0.564 (IV) 


2. The means were found of an observation-series in position 
A and in a corresponding series in position B, in which the metre 


24 
Proceedings Royal Acad. Amsterdam. Vol. ¥ VII 


310 


Was in the reversed position relatively to the observer, i.e. 7 and /. 
In these averages the systematic error is thus eliminated. In this 
way the mean error of one series was found to be 


WILDEBOER Dinprrink BAKHUYZEN Mean 
0.370 0.296 0.507 0.401 . (V) 


If on the other hand a series in position A was combined with 
one in 4, in which the metre was in the same position with regard 
to the observer, so that the systematic error was not eliminated in 
the mean, the mean error was found to be: 


WILDEBOER DinpuriInk BAKHUYZEN Mean 
0.424 0.755 0.768 0.666 . (VI) 


Both the double sets of mean errors (III) and (IV), and (V) and 
(VI) show clearly, that there is a systematic difference in the results 
of the series r and /, or with different positions of the metre relatively 
to the observer. In order to remove the error, therefore, the mean 
of two corresponding series of observations must always be taken, 
in which the metre is in different positions with regard to the 
observer. 

We further computed the mean error from all the series of ob- 
servations for the same portion of the measuring-bar, without regard 
to the position of the metre or of the observer, in which therefore 
the influence is present both of the position of the metre and of 
the observer. First the mean errors were computed for each observer 
separately. This gave 


WILDEBORR DIuPeERINK BAKHUYZEN Mean 
16222 0.805 0.955 1.009 , (VII) 


Finally the results of the series for the same portion of the 
measuring bar in all positions of the metre and of the observer for 
all three observers were averaged, and the mean error determined 
from the deviations of each of the results, which must therefore 
contain (1) the influence of the position of the metre (2) the influence 
of the position of the observer, (3) any other possible influence of 
the observer. The mean error was then found to be: 

15002, 0, on te 2 Se ODL 

The difference of the mean errors (VII) and (IV) shows, that the 
position of the observer has a marked influence, on the other hand 
the agreement of the mean errors (VII) and (VIII) shows, that there 
does not appear to be an influence due to the observer other than 
that which depends upon the position of the metre and observer. 

We may further conclude from the values found, that if the two 
systematic errors mentioned are elimimated, the mean error of a 


oll 


series of observations is the mean of the values: 0.420 (1), 0.428 (IN), 
0.434 (IIT) and 0.401 (V) therefore: 
m— a= O42 

As the measurement of each portion of the measuring bar was 
obtained for each observer by taking the mean of 8 series of obser- 
vations, the mean error in the length of each portion measured by 
one observer is: 

0#.421 
ae Se ea 
V8 
and as the whole measuring-bar consists of four portions, the mean 
error in the length of the bar for each observer is 
UPA (7 4 = SOK 298. 

If the value of this mean error is formed by comparing with each 
other the lengths of the measuring-bar according to each of the three 
observers, we obtain: 

= 0#2355. 

From the agreement of the last fwo values we may conclude, 
that in the results obtained the influence of the observer and of the 
position of the metre and the measnring-bar is eliminated, and that 
therefore, beyond the influence of the temperature determination and 
errors in the coefficient of expansion, the mean error in the length 
of the whole measuring-bar expressed in the length of metre 27, 
determined by one observer, is equal to 

: == (04.36. 
and is therefore for the mean of the three observers: 


0.36 
= — = 04205 
V3 
Geodesy. — “Comparison of the Dutch platinum-iridium Metre 


No. 27 with the international Metre M, as derived from the 
measurements by the Dutch Metre-Commission in 1879 and 
1880, and a preliminary determination of the length of the 
measuring-bar of the French basc-apparatus in mternational 
Metres.” By Prof. H. G. van pe Sanpe BAKkHUYZEN. 


The main object of the measurements made by the Dutch Metre- 
Commission (BosscHa, OvuprMans and SramKart) at Paris in 1879 
and 1880 was an accurate comparison of the two Dutch metres 
19 and 27 with the Métre des Archives, the various papers published 
by Bosscna on the subject show, how very well this object was 

214 


3li2 


attained. As we shall have to refer to these papers more than once 
we shall quote by volume and page from “Bosscua’s Verspreide 
geschriften” (B.’s collected papers) published in three volumes. 

The importance of a comparison of the Dutch metres with the 
International platinum-iridium metre kept in Paris was, however, not 
lost sight of by the Commission. It was probably by their request, 
that in the protocol drawn up of the handing over of the two 
metres by the French Section of the international Metre-Commission 
to the Duteh delegates BosscHa and OvupgEMANs it was specially stated : 
Cette remise est faite sous la réserve du droit qu’aura le Gonver- 
nement des Pays Bas de faire effectuer les comparaisons entre ces 
metres et le prototype du Bureau international des poids et mesures 
pour la determination de leurs equations a VPégard de ce metre. 

However, not only did the Dutch Commission leave open the 
possibility of obtaining a direct comparison with the international 
metre later on, but also by making determinations at Paris of the 
differences between the Dutch metres and metres which are in their 
turn connected to the International metre, they took care, that the 
relation between the lengths of our metres and the International 
metre can be calculated. 

Although all the observations which are required for these caleu- 
lations are fully communicated in Bosscna’s papers and only very 
simple caleulations are sufficient to obtain the relation in question, 
the results have not been published either by Bosscua himself or 
as far as I know by anybody else; and as they are needed in order 
to express the length of our base-line in international metres, I shall 
here shortly communicate them. 

The relation to the International metre is obtained not only through 
the metre des Archives A (see further down), but also through the 
two Metres /, and 20, both of the second alloy of Marrnry, of 
which .J/ is also made; in addition use is made of the two metres 
23 and 27 both of the first alloy (metal du conservatoire). 

For the reduction of the difference of length of 23 and /, the 
difference of the coefficients of expansion of these two metres is 
reqnired, and I shall therefore try to derive its most probable value 
from the results communicated by Bosscna. 

In the first place we may conclude from BosscHa’s calculations, 
that the metres of the second alloy have all got the same coefficient 
of expansion (Vol. III, p. 74—76). The equality of the coetficients 
of expansion of the metres 1, 3, 12, and 13 of the first alloy is 
also demonstrated (Vol. I[l p. 77). According to Fizeau’s measure- 
ments the coefficients of expansion of the metres 19, 27, and 23 of 


the first alloy would also have very approximately the same value 
(Vol. Il, p. 314), whereas according to the measurements of the 
Dutch Commission the difference in expansion of the metres 19 and 
23 is too small to be observable. (Vol. II, p. 314, 315). This is 
not quite in accordance with Fizwau’s results (Vol. II, p. 823) obtained 
at 12°, 42°, and 62°, as these give for 19 and 27 somewhat different 
values. but if the quadratic term is taken into account, the coeffi- 
cients of expansion at 40°, the mean temperature used by Fizvav 
in his measurements, would be according to his formulae 8’.74 for 
49, and 8”.75 for 27, so that in connection with the equality men- 
tioned above of the expansion of the 4 first-named metres of the 
“metal du conservatoire” and the equality of the expansion of 19 
and 23 found by the Dutch Commission it may be inferred, that all 
the metres of the first alloy have also the sume coefficient of expansion. 

The next question is, what the difference is between the coefficients 
of expansion of the first and second alloy. 

According to measurements by Brnorr and GuiLLaume with Metre 
6 of the 2°¢ alloy the mean expansion between O and 20° per 
degree and per metre is 8’.617; according to measurements by 
Fizeau the mean of the same expansion for metres 19 and 2 
the first alloy is 87.537, i. e. a difference of 0.408. It is necessary, 


© i 
however, to observe, that the two values were obtained by altogether 
different methods, that of Brenorr and GuiniaumE by ordinary measure- 
ments of length at different temperatures, that of Fizeau by his 
well-known interference-method. 

Against these we have the determinations of the differences in 
expansion of metre 6 of the 2°¢ and of metres 1, 3, 12, and 13 of 
the 1s* alloy (Vol. IIL p. 77) all from ordinary measurements of 
length at different temperatures. As the result of these 0”.02 is 
obtained as the average of the differences. 

Taking into account, that, where the methods of observation differ, 
systematic errors in the differences are possible, it seems to me 
probable, that the latter result is the more trustworthy. 

In the reduction of the Dutch metre 27 to the International metre 
the difference in length of metres 23 and 27 also plays a part. 
For this difference two values have been determined; in 1879 the 
Dutch Commission found 27 — 23 = 0.92 + 0*.031 (Vol. I, p. 297) 
and in 1880 the same commission found 27 —- 23 = 0.41 + 07.073 
(Vol. If p. 334). Of the latter value no further use has been made 
by Bosscua; it seems to me, however, that it is preferable to use 
the mean of the two results, taking into account the respective 
weights. In that case the result is 


Reduction by means of I,. From several series of observations at 
a’ mean temperature of 16°.44, Tresca found (Vol. III, p. 14) 
23 = J, + 14.24. 
Adding 0°.02 < 16.44 = 07.33 for the reduction to 0° the equation 
becomes 


93 = 1, 1657, 


further 27 = 23-+ 0.84 (see above} 
and I, = M- 5.94 (Vol. Ill, p. 70), 
so that 27 = M+ 8.35. 


Reduction by means of 20. From three series of measurements 
one by Bosscua and two by Tresca, follows : 


23 = 20 + 7#.19 (Vol. III, p. 24), 


further 7} ee 23 ais Or. can (see above) 
and Fol. Til, pesto} 
so that 27 = M 4 8.99. 


The mean of the two reductions is 27 = M+ 8+.67. 

If the 5 above mentioned different equations containing 4 unknown 
quantities, are taken as all equally accurate and if they are then 
solved by the method of least squares, obviously the same value 
for 27—JV is found, while the mean error of each of the equations 
is + 07.32, that of 27 — 17 =8".67 being + O?.45. 


A value for 27— J/ is also arrived at by using the comparisons 
with the “Metre des Archives’ A, viz. 
27 = A+ 64.11 (Vol. II, p. 323), 
A=M-- 2.63 (Vol. Ill, p. 24). 70); 


Hence 27 —M+ 8.74. 

This result agrees very closely with the value found above. But, 
as it is largely based on the comparisons which have also served 
for calculating the previous result, no particular importance can be 
attached to the accordance. Considering the value of the mean 
error + 0.45 a direct comparison of 27 and WV would certainly 
seem to be desirable. 

If the length of the measuring bar of the French base-apparatus 
in terms of metre 27, as given in the previous note, is now expres- 
sed in International metres by means of the equation 27 = J/ + 87.67 
the result is; 


L=4 M— 391-84 + 4 & 84.67 =4 M — 3574.16. 


The value of Z had been determined several times before at the 


“Bureau international des poids et mesures” at Breteuit; on these 
occasions the following values were obtained, leaving out the some- 
what uncertain correction for the “change in the molecular equilibrium”. 


1903 March 4 M—277".6 Breteuil 
1904 June —-373 .5 re 
1907 February —-363 .7 is 
1909 February. —356 .8 7 
1909 December —358 .4 3 
1910 December —— St ae - 
1911 June 515) a) “ 
1911 Sept.-October - 398 .4 ; 
1913 April —348 .7 “ 
1913-14 Dee.-January —357 .2 Delft. 


It appears from these numbers that during the first years up to 
1909 the bar increased in length. From that year onwards the length 
seems to have remained practically unchanged; only in April 1913 
a further very marked increase in length shows itself, of which, 
however, no trace is found in the measurement made by us. In 
view of this contradiction a new determination at Breteuil of the 
length of the measuring-bar is desirable; col. LALLEMAND, chief of 
the geodetic department of the Service géographique de l’armée, and 
Monsieur Bunorr, Director of the Bureau international des poids et 
mesures at Breteuil, have both promised to undertake this comparison 
shortly. 


Postscript. A few weeks after the meeting of our Academy 
I received from Monsieur benoit a letter in which he communicated 
the results of an elaborate investigation concerning the length of the bar 
of the French base apparatus. He and Monsieur Mauprer compared 
in the Bureau at Breteuil first that bar and three other ones each 
with the prototype and afterwards the four bars with one another. 
Benoit found as final result for the length of the French bar, with- 
out correction for the change in the molecular equilibrium: 

L, = 4 M — 3487.23 , 
almost exactly the same value as that found in April 1915. 

On the average the length determined at Breteuil is therefore 8’.7 
greater than that determined at Delft. 

In order to find what may be the causes of that difference I 


316 


used the formula by which the length of the bar at zero is derived 
from the measurements. 

During the measurements at Breteuil the temperatures of the bar were, 
according to Brnorr’s statements, not very different from 15°. I bave 
not here at my disposal the data of the exaet values of the tem- 
peratures during the measurements at Delft, but I know that they 
presented no great deviations and, if I am not mistaken, the extreme 
differences from the mean, about 15°. were not greater than about 
two degrees. We can therefore combine the observations at Breteuil, 
and also those made at Delft each into a mean result, at a mean 
temperature, and we then obtain the following equation, in which 
the letters without a dash indicate the values determined at Breteuil, 
those with a dash the values determined at Delft: 
Lp=L tel, T=4l,+48t+S8 , p= +e'Lh | T’=41,'+48t-+S, 

L,— bhi eh, Fee Ll Poe AG 1) 468) ae 

In these formulae Z is the length of the bar, 7 its mean tem- 
perature during the measurements, « the adopted coéfficient of expansion 
of the bar, / the length of the comparison metre, ¢ its mean tem- 
perature, 3 the mean expansion of the metre for 1°, S the difference 
of the length of the bar and the fourfold of the length of the com- 
parison metre, determined by means of micrometrical measurements 
with the microscopes; 7’ and 0, as indices of LZ and / indicate the 
temperatures to which these lengths have been reduced. 

The differences of the temperatures 7’— 7” = AT and t—t = At, 
and also the differences in the adopted coefficients of expansion 
8— p'=Ap are small, and for the value of the coefficient of ex- 
pansion «@ and e« the same value has been adopted in Breteuil and 
in Delft; the last of the three equations may therefore be put 
approximately into the following form: 

L,— LL, =4L=—aLAT+ 4Al 4 4pAt 4+ 4tAg+ S—S’. 

When A7’, At, Al, As and S—S’ have their exact values, AZ 
is zero; the value 8.7 for ASL found from the observations is there- 
fore only a funetion of the errors in those values, and putting on 
the first side of the formula AZ = 8’.7 the quantities on the second 


side represent those errors. We will consider each of the terms 
separately. 

1. «LAT. T and 7” have been determined in the same manner 
by readings of the thermometers laid on the surface of the measur- 
ing bar within the thick aluminium case; the temperatures in both 
comparators were fairly constant, and the value of @ is small; eZ 
for O°. is about 07.7. In view of the great value of AZ, we may 
therefore neglect that term. 


317 


2. S-—S’. Taking into account the precision of the micro- 
metrical measurements and the small influence of the systematic errors 
in the measurements made at Delft, as appears from the values of the 
mean errors, that term may also be neglected in trying to explain 
the great value of AL. 

3. 484¢. 43 is about 34” and Af is the difference in the errors 
of the mean temperatures of the metre, determined at Breteuil and 
at Delft. When we assume, that in the perfectly constructed 
comparator at Breteuil the error in the mean temperature of the 
metre was zero, the effect of an error of 0°,1 in the mean tempe- 
rature of the metre at Delft on its length is 3”,4, and in order to 
gel a positive value of AZ the temperature of the thermometer 
laid on the surface of the metre must be lower than the tempe- 
rature of the metre itself. 

During the measurements the temperature of the metre was slowly 
rising, it is therefore improbable, that the teimperature of the thermo- 
meter should be systematically lower than that of the metre, and it 
is difficult to explain the positive value of AZ, either totally or for 
the greater part by an error in Af. 

4. 44/7. I cannot say, what is the real value of A/, the error 
of the difference I adopted between the length of metre N°. 27 and the 
International metre.. The mean error of the adopted value of 44/ 
is +1”.8. It is therefore possible that a part of the AZ may be 
accounted for by an error in the adopted difference, but it is 
improbable, that it should explain the whole value, 8%.7 of AZ. 

5. 4t43. We can determine a fairly probable value of that 
term. According to a telegram from Monsieur Brnorr, the mean expan- 
sion for 1° between O° and 15°, used in the reduction of the 
measurements of the prototype, made of the second alloy, is 8’,662, the 
mean expansion per degree between the same limits adopted in my 
reductions of the length of N°. 27 made of the first alloy is 8’,493 ; 
the difference between the two is 04,169. As a_ result of direct 
comparisons, the mean difference of the expansion of the metres of 
the first and second alloy is 07,02, as I stated above. 

If we assume, that the coefficients of expansion of the metres 
of the second alloy are really equal and that it is the same with 
the metres of the first alloy, which assumption after the researches 
of Bosscna is very probable, the error 43 would be equal to 0.169 
—(0.02 = 02,15. As ¢ is about 15°, the term 4¢Af is 9”, almosi 
equal to the value 87,7 found for AL. 

Although I do not pretend, that the assumptions made in order 
to explain the difference between the results obtained in Bbreteuil 


318 


and Delft are absolutely certain, still I believe that the probability 
is not small, that the difference between the assumed and the real 
coefficients of expansion of the prototype at Breteuil and the 
metre N°. 27, is for the greater part the cause of the value of 
AL. It remains absolutely uncertain, what the real coefficients of 
expansion of the metres are and also whether the coefficient of N°. 27, 
determined after Fizuavu’s method, merits greater or less confidence 
than that of the prototype deduced, as I believe, from direct measure- 
ments at different temperatures. But whatever it may be, it is of great 
importance, and it is in my opinion the chief result which may 
be deduced from my discussion, that when a direct comparison 
of the metre N°. 27 and the international metre shall be made, 
according to the right given to our government, it will not be confined 
to a comparison at a mean temperature, but that if possible, the 
absolute coefficient of expansion of our metre, and certainly the 
difference in expansion of N°. 27 and the prototype will also be 
determined. 
Lenk (Switzerland. 


Physiology. — “On the formation of antibodies after injection of 
sensitized antigens.” Il. By Dr. L. K. Worrr. (Communicated 
by Prof. C. Eyxmay.) 


I. As a continuation to my series of experiments given in the first 
communication, | have examined the immunisation power of a mixture 
of erythrocytes and specific serum with a surplus of amboceptor. 

It is generally stated in literature that this power is very slight or 
that it does not exist at all; in my two series of experiments I have also 
found very little or no formation of amboceptor. I shall communi- 
cate one of the series. 

Horsecorpuscles — specific rabbitserum */,,, strong. 

Binding power of 1 ecm. 5°/, blood + 7 doses. 

Mixture of 40 c.em. serum and 20 e.em. undiluted blood i. e. 
20 doses amboceptor, so a great surplus. 

Rabbit 149, 73 and 76 each get 20¢.em. of the mixture intraperitoneal. 


x, ADS Oennavelecale =, - 6'/, ,, undiluted blood only % 
Titre after 1 day after 7 days after 12 days 
149 Yi) weak ae Ear 
(i aif 1/,, weak 1/,, weak 
76 “ie ‘/,, weak ha 
179 7s ia “en 
70 aa iNet Woon 


@ re “Laoo AGE weak, 


319 
/ 

So with the rabbit 149 and 73 we do not find a trace of active 
immunisation, only of passive; rabbit 76 after 12 days shows a 
small (active) increase of titre. The controlling rabbits however have 
distinetly formed amboceptor. 

The second experiment with cattle corpuscles had a_ perfectly 
analogous course. With these experiments we cannot inject intra- 
venously; the animals which are intravenously injected with such a 
great quantity of serum and corpuscles die of anaphylaxis. 

II. I have now put to myself the question what happens with 
the sensitized corpuscles after the injection into the rabbit or cavia. 

Therefore | have for the time being confined myself to the sub- 
cutaneous resp. subconjunctive injection; the intravenous one is very 
difficult to follow, the progress of the peritoneal one it mostly known ; 
besides the subcutaneous is the only one that is to be considered 
with regard to man. I expected that in keeping with what happens 
in the peritoneum, viz. a solution of the sensitized red corpuscles 
in a short time, the corpuscles would also dissolve in the subeuta- 
neous tissue. I have taken the conjunctiva as the spot where to 
inject: there the phenomena are to be controlled better than any- 
where else, and one can easily cut out little pieces for microscopic 
examination. 

Well then: if we inject foreign corpuscles under the conjunctiva 
they are generally gone after one, and certainly so after two days. 

As they have no movement of their own, we must assume them 
to be led away along the lymphpaths a leading away by phago- 
eytes in such a short time is not to be assumed. It is however 
different if sensitized corpuscles are injected; these remain on the 
spot; they do not dissolve in any quantity worth mentioning, and 
if one microscopies the place after a longer or shorter space of time 
(after cutting out, fixing, embedding, and colouring) one will find 
an important number of leucocytes between the corpuscles. 

After 6 to 8 days only the corpuscles have generally disappeared; 
sometimes however they are still to be seen after 10 to 12 days. 

During the first few days one mostly finds polynuclear small 
leucocytes, later more great mononuclear ones. 

Now the question is how to explain this conduct. For this we 
must examine three things. 

Ist. How is it that the sensitized corpuscles which are injected 
subconjunctively do not dissolve, while those injected intraperiton- 
eally do. 

2nd, Why do the sensitized corpuscles remain in the same place, 
whereas the normal ones are carried away. 


320 


3°'. What happens finally to the sensitized cells; what do the 
leucocytes do. 

Let us first answer the first question. 

Here we must ask at once if there is complement in the sub- 
cutaneous lymph. 

As far as I know H. Scuneiper’s') researches about this subjeet 
are the best; he found that the tissue lymph which is obtained by 
bringing a piece of cottonwool under the skin, and afterwards 
pressing if out, contains very little complement indeed. One always 
finds a littlke more complement than would really be the case if 
we had pure tissue lymph; a slight mixing with serum can of 
course hardly be avoided. It goes without saying that in this 
Way we cannot be certain to get a liquid, agreeing with the tissue 
lymph; the piece of cottonwool naturally works irritating; an 
inflammation arises. But the injection of the corpuscles also causes 
an inflammation, and as such these two processes are equal. 

I have also made some complement titrations to the guinea pig 
and rabbit, of subeutaneous fluids obtained in this way. 


For the solution of my haemolytic system I needed : 
1/ 


I. Fresh guinea pig serum Hori Gitte 
Subcutaneous fluid “om Cxe lta. 
[I]. Fresh guinea pig serum eeGRC NN: 
Subcutaneous fluid Win (OsK0e 
Ul. Fresh rabbit serum Wf, CxO. 
Subeutaneous fluid 0,6 c.cm. no haemolysis ! 
Siowing fluid 0,6 c.cm. trace of ,, 


So we can affirm ScuNemeEr’s experiments and assume very little 
or no complement to exist in the subeutaneous cellular tissue ; and 
we need not be astonished about the sensitized corpuscles not dis- 
solving, when being injected subcutaneously. 

Now we must answer the second question. The sensitized cells 
remaining in the same place was supposed to be due to the agglu- 
tination which always accompanies the sensitizing. I did not succeed 
in obtaining an immune serum prepared in the usual way, which 
did not at the same time agglutinate. As I did not know any 
method to separate amboceptor and agglutinin when I started my 
experiments, | took another way to prove that the remaining of the 
bloodcells was owing to their being agelutinated and not to the 
sensitizing. | therefore agglutinated the bloodecells in a different way, 
and now found that clinically and histologically the same was to be 
seen after injecting these corpuscles as after injecting sensitized (and 


1) Arch, f. Hygiene 70. p. 40 seq. 


321 


at the same time agglutinated) cells. In the first place T used a 
colloidal solution of SiQ, for it. 

All the red bloodcells I used (rabbit, guinea pig, horse, cattle, dog) 
were agglutinated by it, be it in various concentration. Only the 
SiO, had no effect; it caused neither swelling, nor leucocytosis. It 
had been prepared by saponifving Siliciumethylether (Itan_BauM) with 
greatly diluted hydrochloric acid. Colloidal SiO, prepared in a different 
way had the same effect. Now one might object against this 
experiment that the SiO, not only agglutinates the bloodcells, but 
that it also sensitizes them; for together with guinea pig serum ina 
great quantity, it can dissolve some kinds of blood. Therefore I took 
refuge to the vegetable agglutinins which are found in the bean, 
pea, lentil, and in the seeds of Datura Stramonium. In all these 
cases the result was the same: the bloodcells always remained there ; 
the conjunctiva also showed the wellknown bluish-red change of 
colour after some days, and histologically the image was always the 
sane. It goes without saying that with all those experiments the 
sterility was taken into consideration as much as possible. *). 

In order to make quite sure, however, that only sensitized and 
agglutinated corpuscles did not show the phenomenon, I examined 
some thirty rabbits out of my collection on haemolysin and agglu- 
tinin against sheep-erythrocytes, and I really found some sera which 
did contain baemolysin, but only little agglutinin. I repeated the experi- 
ments with these sera; but the results were not very distinct : there 
sometimes was a difference, but it was not big enough to draw a 
certain conclusion from it. 

This is because all the sera employed were rather weak (ambo- 
ceptor */;,—'/,9.) and so a rather big quantity of serum was necessary 
(+ 3 em.) to sensitize the cells. Normal rabbitserum generally con- 
taining some agglutinin, we did not sueceed in this way in obtaining 
a suspension of sheep-erythrocytes which are sensitized but little or 
not agglutinated. Yet I ean communicate one experiment which came 
out rather well: 

Serum rabbit 73 titre amboceptor ‘/,, very little agglutinin. 
cml tt! 87h o, oe srneanly a>, much iy 


» 100 


1/, ecm. sheep-erythrocytes is digested with += 3 cem. serum 73, 
just as ‘/, ecem. with +3 ecm. serum 147. The suspensions are 
centrifuged and the corpuscles are taken up in 1 cem. saltsolution. 
Erythrocytes 73 are injected on the right, erythrocytes 147 on the 

1) I did not use ricine because the poisonous qualities of this substance would 
have injured the image. 


322 


left under the conjunetiva of rabbit 172. The serum of this rabbit 
contains neither amboceptor nor ae in a noticeable quantity 
against sheep-erythrocytes. 

After one day there is a distinct difference. There is very little 
swelling and redness (+) on the left, but very strong swelling and 
bluish-red change of colour (+-+-++) on the right. The next day the 
difference is a little less, but still it is distinet. 

Consequently it was desireable to obtain a serum which sensitized 
strongly (at least ), but whick agglutinated little or not at all. 
As there was no question of a chemical separation — all the litera- 
ture tells us that all suchlike attempts lead to no result whatever — 
such serum had to be obtained in a different way. In the literature 


1000 


about the heterogenetical antibodies is mentioned that serum of a 
rabbit which had been in some way prepared in order to get hetero- 
genetical amboceptors against sheep-erythrocytes, would then contain 
no more agglutinins than are found in normal rabbitserum. 

My experiments in this direction have however not yet led to the 
desired result. One rabbit which was injected with pempeie 
had a serum with titre '/,,, against cattle-corpuscles, and a titre */, 999 
against sheep-corpuscles. Hoa eet it very clearly contained agelutinins 
against the latter. The same thing appeared with two rabbits which 
had: been injected with horse-kidney extract. The titre against sheep- 
blood was ‘/,,, of both of them. Both distinctly contained agglutinins, 
if only little. The sheep-corpuscles treated with this serum remained 
for some days in the same place, after having been injected under 
the conjunctiva. 

So in this way I could not prove awith certainty that the agglu- 
tinin is the cause of the prepared corpuscles remaining under the 
conjunctiva, * 

11. I will now mention some experiments which have been made 
in connection herewith, but which do not directly bear upon the 
subject mentioned in the title. | have asked myself whether the same 
difference as is mentioned above, is also found when non-prepared 
bloodeells are injected subconjunctively partly with prepared, partly 
with non-prepared animals, and whether here too the agglutinin was 
of any importance as to the remaining of the erythroeytes. And this 
has indeed appeared to be the case. 

Rabbits with serum containing amboceptor (and agglutinin) still 
show a strong swelling under the conjunctiva after one or two 
days after having been injected with the erythrocytes in question 


) Note added during to the correction: Now | had more success with this 
experiment. The heterogenetical serum which | now used was '/aoo9 strong. 


oe 


(in my experiments they were horsecorpuscles), whereas the controlling 
animals showed hardly any swelling after one, and no swelling at 
all after two days. In accordance with this the tissue fluid (obtained 
in the above mentioned way with cottonwool) obtains amboceptor 
as well as agglutinin, if they are in the serum. 
Rabbit 160 immunized against cavia-erythrocytes. 
Serum agelutination '/,, amboceptor ‘/,, weak (+--+) 
fluid * oe * ay key aie 
Rabbit 192 immunized against horse-erythrocy tes. 
Serum agglutination */,, amboceptor 
jluid 3 1/7, weak ,, 1/,, nearly 


/ 
/20 
Rabbit 147 immunized against cattle-erythrocy tes. 
Serum agglutination ‘/, amboceptor */,, 
fluid 1 mie ms lee 
I have now investigated if it really is the agglutinin which deter- 
mines the difference. 


Rabbit 116 agglutination strong, amboceptor ', 


100° 
Rabbit 148 » very weak, fe eee 
Both rabbits are subeonjunctively injected with '/, c.em. washed 


sheep-ery throcy tes. 

After one day there is a very strong bluishred swelling with 116, 
with 148 hardly any swelling; after 2 days still a strong swelling 
with 116, with 148 nearly all the blood has disappeared. 

A stronger proof is given by the rabbits that were injected with 
horsekidney extract’). Although the titre against sheepcorpuscles was 
not high here (with both */,,,) a great difference was stated with 
the controlling animal (titre also */,,,). 

After one day hardly any blood was to be seen with the first, 
contrary to the controlling-animal. 1 think these experiments are 
of some importance. For in the latest great report about the 
agelutination known to me, that by Patraur*), the author says on 
p. 515: Ob Agglutination auch im Organismus stattfindet erscheint 
recht zweifelhatft. 

At least I believe I have proved the haemagglutination to take 
place in the subcutaneous tissue. [| only want to insert bere that 


1) These are the same animals as were mentioned above: their serum did 
contain agelutinin, but much less than the animals immunized in the ordinary 
way. That here we get no agglutinin effect, and that we did when mixing the 
serum with the bloodcells in vitro, may be explained by the fact that the agglu- 
tinin can pierce with so much more difficulty into the tissue fissures and reach the 
bloodcells than when a great quantily of serum in vitro ts directly added. 

2) Kotte und Wasserman, lle Auflage, Il, p. 483—654. 


324 


the phenomena mentioned above belong to the department of local 
anaphylaxis (Phenomenon of Artuus). As far as 1 know they have 
not been studied as to the immunisation with bloodeells; they have 
with serum or bacteria. This really is only a question of name 
however: the essence of local anaphylaxis is still as unknown to 
us as that of general anaphylaxis. 

In any case we can see by the bloodcells that the disintegration 
of albumen is a very slow one; I do not wish to deny however, 
that part of the flood of leucocytes is owing to this disintegration. 
What has been stated somewhere else viz., a primary necrosis of 
the tissue and after that an infiltration of leucocytes '), I have never 
observed; I could sometimes also state a toxical influence of the 
injection out of an oedema of the cornea: but this happened very 
rarely. Then one should not directly compare the phenomena of 
subeutaneous injection with those of intracorneal injection (WESsSELY, 
von Sziny); in the latter ease the current of fluid is much slower, 
so that great differences can occur by this. It would however lead 
us too far if we entered into this more closely. 

We must now still treat of the third question: what happens to 
the sensitized (agglutinated) cells, and what do the leucocytes do in 
this process? I must first of all mention that 1 could not find any 
difference between histological images when injecting sensitized or 
only agglutinated bloodeells. ‘This, however, is in keeping with 
other experiments. For, there being a great difference in vitro between 
the phagocytosis of sensitized (opsonized) and nonsensitized cells, -— 
the former are phagocytated, the latter are not, when brought 
together with suitable leucocytes — one does not find back this 
difference in vivo when injecting the cells into the abdomen, 
previously injected with broth. AcHarp and Forx’*) some time 
ago tried to find the causes of this difference, but in vain. I did 
not succeed either*). We need not be astonished however, when 
finding the same conduct in the subcutaneous tissue as in the 
prepared abdomen. 

Are the erythrocytes now phagocytated? Notwithstanding my 
observing a great many preparations, I did not succeed in getting any 
certainty whatever about this in my histological sections; to form 


1) H. Fucus und Metter, Z. f. Ophthalmologie. Bd. 87, p. 280. 

2) AcwarpD and Forx Arch. de Medecine expérimentale et d’anatomie Patholo- 
gique, January 1914. 

3) Prof pe Vries advised me to add to the mixture (foreign bloodcells, fresh 
serum (without opsonins) and leucocytes) scrapings of the peritoneum endothelium; 
with this | had no suecess either. 


325 


an opinion about it is, however, very difficult; leucocytes are always 
among a great number of red cells and the sections are always 
thicker than one red or white cell. Anyhow, it seems very probable 
to me that this must happen. For: 

1. the red cells disappear atter 6—8 days. 

2. in vitro they are easily phagocytated. 

3. The subcutaneous cellflaid and the leucocyte extract do not 
contain an unspecific haemolysin (ScuNumwer: |. ¢.; this concerns 
polynucleous (mikrophages) as well as mononucleous cells (macrophages). 

I have tried after one or two days to cut out the swelling (after 
injecting the sensitized (agglutinated) cells), and then to spread them 
out on a coverglass: these preparations too gave bad images; princi- 
pally by the stickiness of the substance: I did not see a distinct 
phagocytosis. 

I have here always spoken about sensitized cells without wishing 
to form an opinion about the open question of identity between 
amboceptors and opsonins and tropins. (NEUPELD *) SaTSCHENSKO’’) ). 

The following experiment will show that there can be amboceptor 
as well as tropins in the subcutaneous cellular tissue. A piece of 
cottonwool was entered under the skin of the abdomen of a prepared 
rabbit (against sheep-erythrocytes) and the fluid was examined after 
some hours: in vitro it sirongly stimulated the phagocytosis of 
sheep-erytrocytes by rabbit-leucocy tes. 

As a summary we can draw the following conclusions: 

1. When using red corpuscles loaded with amboceptor as antigen 
one should remove all surplus of serum. 

2. Sensitized and agglutinated red corpuscles, when injected sub- 
cutaneously, remain in the same place for a long time; non-treated 
cells are soon led away. 

3. This will most probably be the consequence of the agglutination, 
not of the sensitizing. The same happens to non-specific agglutination 
— also when it concerns the animal’s own cells. 

+. With prepared animals possessing agelutinin, the cells injected 
also remain in the place where they have been injected. So agglu- 
tination in vitro also takes place; this is not the case with animals 
which only possess amboceptors (opsonins) and no agglutinins. 

5. The subcutaneous lymph contains very little or no complement, 
it does contain amboceptor, agglutinin, opsonin (tropin). 

The above will show my experiments not yet to be complete. 
They require to be completed as to the question to what 
“1) Arbeiten aus den Kaiscrl. Gesundh. Bd. 25, 27 en 28. 

*) Arch. Se. biol. St. Petersburg. XV, blz. 145 1910. a 

Proceedings Royal Acad. Amsterdam. Vol. XVIL. 


extent the immunizing power of red corpuscles loaded with antibodies 
is related to that of normal cells as to the tropin- and the agglutinin- 
content of the serum. We may suppose, also in consequence of the 
above mentioned experiments, that the content of antibodies of serum 
and subcutaneous lymph goes parallel and so we shall not investigate 
this point separately. 

IV. After the immunisation with sensitized erythrocytes the one 
with mixtures of serum and anti-serum comes next. I have not 
stated the amboceptortitre (to be stated by means of complement 
fixing) but the precipitincontent. Where the results do not differ 
much from the experiments with sensitized erythrocytes, 1 think I 
can suffice with only stating the precipitin. 

7A Rabbits, injected intravenously with horseserum, 0,5 ¢.c.m. per 


ke. (made inactive). 
> 


Rabbit weight titre after 3days after 5 days after 7days after 12 ds. after 14 ds. 
103 26007 3 =— of z Pa t= ae s} "oo hoo 
104 2850 — lB ee =) \s | — NE EF Yoo weak — /r900 
105 2830 i Ne a A 7 2 ¥ — 5 - Thooo » "/r000 
106 1650 tS Zs vee z\ he x "hoo “/iooo Weak 
107 2100 — a8 = pe SI Mio) weak Th o00 


/B. Rabbits injected, intravenously with 0,5 ¢.em. horseserum 
(inactive) + 1 ccm. precip. serum ('/,,,,), after this mixture had 
stood for 1 hour. 


Rabbit weight titre aft. 3days after 5 days after 7 days aft. 12 days aft. 14 days 


8 = 2150 — ges —(og “ho "hoo Yoo 
109 2150 = 5 5 5 — E 5 ho Thooo Miooo 
a ee — ie 2 © et par = ae some . ‘hoo ‘A000 
35 = at ys — ea te — (horse serum 
5 a fellas /ho00 / 1000 
112 9150 — et = s /ip Weak Mhogo weak 1/009 
So here we do not see a distinct difference between the A and B 
group. 
Il A. Rabbits, injected intraperitoneally 0,4 cem. human serum 
>} * 
per kg. 
Rabbit Weight after 5 days aft. 7 ds. aft. 10 ds. aft. 12 ds. aft. 14 ds. 
67 2150 — g ; “= tho 000 Mhonoo 
78 2450 — 5 5 = hho hoo T/1o99 Weak 
70 1900 — /s 5 = Vio ooo 1 0000 
60 2320 — jog Wo? 1/00 1 000 M1000 
76 1820 — a 1h hoo hoo 10000 


II B. Rabbits injected similarly 0,4 eem per keg. + 3.6 cem. 
antiserum (‘/,,,, largely). The mixture had stood for 4 hours, a thick 
precipitate has been formed. 


O26 


alt. 7 dss atte VONdss © Jatt) 12) ds. “aft. 14 ds: 


9 
=) 
or 
a 
7 


Rabbit Weight 


2100 —— 5 \ - hoo “hooo 1000 
114 3200 — (: 2) = = = “ho 
113 2000 — /¢§ i ; = = et tho 
112 2550 —_ (2 :| = =a “ooo "/igo Weak 
7/Al 1600 pil = Te a 1h ooo 1/0000 


After 17 days the titre already went back. 

Here we can see that, whereas of the series B three rabbits 
distinctly lag behind, two of them reach as high a titre as the A 
rabbits. Knowing (UsLENAUTH) that accidental failures in the preparation 
of precipitinholding sera are not to be avoided, I should not wish to 
draw any other conclusion from this than that a good formation of 
precipitins is also possible with mixtures of serum and antiserum. 

I have also taken the following series of experiments. 


III. Rabbit 140 1 c.cm. horseserum intraperitoneal. 


ee kG * 5 » + 1 cem antiserum 
(*/1000) 
» 142 - ‘ Sng crt, Sha ss 
e 99 33 An Wey SIMO! Gata 
Perio teas OO 7? este oe 
7: 8 2 0 Diet! Ae 
i 42 5 x ad foter dy MES, 
es 48 3 93 Geeta OV ee 
Rabbits after 8 days 
140 oe 
116 ‘Tipo 4Wweak. 
142 a epaiate Mn 
v9 Hitent 
121 t/acus 
8 piaaen 
42 aetet 
48 — 


So here too we find a rather important formation of antiserum 
with rabbits, which, with the serum, bad also got antiserum. 


IV. Rabbit 155 50 ¢.em. antiserum ‘/,,,, -- 2¢.cm. horseserum intraperil. 


per is6: 30, ‘ Fiat alae 
57 10) | ‘ nae ‘ 
marissy On, 3 ia) a : 
meson dS. .. y ae ; i 


328 


Rabbit after 1*/, hour after 1 day after 3 days after 5 days 
contains — | » contains / contains / contains 
es se serum | horse serum horse serum horse serum 


dd - —\+++4¢—\) ++ + 
156 Sie aby a ge ++ 


as, oy < — eee z 4? 


Pah ae shaRAE = aioe ++ 


169 aes : 


after 7 days. aft. 10 ds. aft 12'ds. att. 4vdse Vath diadee 


contains 
horse serum 28 
aos 
Sk <> 1/ 1) . 1 
155 = + ailing BS 5 100 /1000 Ww. nee 
LOG Staats > IE a 3 > ‘L100 weak L100 WwW. “hres 
Si | 1/ oe) 1 9 1 
157 — — fio a oa : ho Ww. 
KO 1/ Aes / 1 1/ 
158 — staat 10 3 a /100 /100 /100 


1G eee re a ee ve om 


Here too we also see some irregularity: (rabbit 157 immunizes 
somewhat less than the other, but even a mixture of 25 times more 
antiserum than serum still has immunizing: effect. 

I did not try if surplus of serum can do any harm when 
immunizing, for one then gets too great quantities so that it is hard 
to inject them: 50 ccm. serum is rather much for a rabbit. 

These experiments seem to be somewhat contrary to a communi- 
cation of Do6rr (report about Anaphylaxis, Kote unp WassrrM. 
Ile Aufl.), that the precipitate obtained by mixing serum and _ anti- 
serum, has no immunizing effect. But this is only a seeming 
contadiction. For, according to investigations e.g. by Wetsa and 
CHAPMANN’) this precipitate only contains traces of parts of the 
serum and it is almost exclusively formed out of the antiserum. 

Thus I have found that of a serum of a rabbit which was 
immunized against human serum (titre '/,,,.) 75 ecem. was necessary 
to form together with 1 cem. human serum (together till 150 cem.) 
a precipitate, so that in the above mentioned liquid no more human 
serum could be indicated with my antiserum (’/,,,,). 1 cem. being a 
very small dosis to immunize a rabbit, it is clear that not much 
can be expected in general from an injection of the precipitate’). 

I have now also examined the local effect of serum and antiserum. 


1) Zeitsch. f. Immunitiitsf. 9, p. 517. 
2) T here give up the question whether there is any human serum at all to be 
found in the precipitate, or whether it could be again removed by washing. 


329 


With this the antiserum and serum were always both inactive, so 
that we have nothing to do with any possible anaphylatoxin. 

If one again injects the mixture in which a precipitate has been 
formed subconjunctively, one will find a rather strong swelling the 
next few days, which at a morphological examination again seems 
to contain polynucleous cells. The controlling animals which had 
only been injected with serum, were normal again the next day. 

If one centrifuges the mixture, the above mentioned liquid is not 
found to cause a swelling, but the precipitate is. So we have here 
an analogous conduct as with the corpuscles’). 

I have now tried whether specific albumen precipitations did not 
show the same conduct, and for this I chose the precipitates of 
horseserum with colloidal He (OH), and S/O,. Both precipitates 
gave some swelling and ata morphological investigation polynucleous 
Jeucocytosis. This investigation must still be extended. 


If one injects a prepared animal with specific serum, one gets 
the same phenomenon: swelling and lencocytosis. This phenomenon 
is wellknown. I did not yet succeed in proving here as well that 
the precipitins hold the serum in its place’*), although | do think it 
likely, considering what goes before. For the time being I do not 
see a chance of preparing a serum which possesses amboceptor 
against foreign albumen, but no precipitin. 


Amsterdam. Path. Anat. Laboratory of the University. 


Chemistry. — “The Temperature-coefficients of the free Surface- 
energy of Liquids at Temperatures from —80° to 1650° C. 
1. Methods and Apparatus. By Prof. Dr. F. M. Janeur. (Com- 
municated by Prof. P. van Rompuran). 


§ 1. The purpose of the experiments here described was to en- 
deavour to ascertain the relation between the so-called “molecular 
a relation 


surface-energy” of molten salts and the temperature, 
which has hithertho been studied only in liquids, which possess no 
electrolytical conductivity. 


1) The experiments are somewhat analogous to those about the local effect of 
the anaphylatoxin (fRiepBeRGER), but I always used serum that was made inactive, 
contrary to the investigators, into the anaphylatoxin. 

2) That is to say subconjunctively. For the cornea other laws probably prevail; 
there the serum remains in the same place for rather a long time without there 
being any precipitins (WersseLy, von Sziny). 


330 


A probable relation founded upon the law of corresponding states, 
between the value of the temperature-coefficient of the expression : 
Ge) , and the degree of molecular association of a liquid was 
first suggested by Eérvés*), and later by Ramsay and Saietps*) and 
a number of others*). These observations appeared to prove, that 
the values of these coefiicients do not differ much from 2,2 Erg 
per degree C. for “normal” liquids, while for associated ones they 
are considerably less. In any event some definite knowledge of the 
dependence of the free surface-energy x upon the temperature will 
be of high importance for the consideration of all problems, relating 
to the internal state of liquids. 

It can hardly be supposed with any probability, that the law of 
corresponding states will be found to apply in the case of molten 
salts, because they are really electrolytes and more or less dissociated. 
Notwithstanding this, if the investigation should chance to reveal 
relations in any way analogous to those hitherto supposed to be 
characteristic of organic liquids, this fact must carefully be considered 
in estimating the significance of the theoretical speculations mentioned, 
and especially is this the case, where criteria are sought for judging 
about the molecular state of liquids in general. In fact, one can 
better hope to elucidate the influence of chemical constitution on 
characteristic properties in the case of molten salts, than in the ease 
of the much more complicated organic molecules. 

These and other considerations, some years ago (1910) suggested 
the development‘) of an experimental method, which should permit 
the study of the dependence of the molecular surface-energy upon 
iemperature, — even up to temperatures in the vicinity of 1650° C. 

1) Kérvés, Wied. Ann. 27. 448. (1886); vAN DER WAALS, Zeits. f. phys. Chem. 
13. 713. (1894). Erste. Ann. d Phys. 34. 165. (1911-) 

2) RAMSAY and Surewps, Zeits. f. phys. Chemie 12. 483. (1893). 

8) Vid.: Guyz and collaborators, Journ. de Chim. phys. 5. 81, 97. (1907); 9. 
505 (1911); etc.; WaLpEen and Swinney, Zeits. f. phys. Ghem. 79, 700. (1912) 
3ull. Acad. St. Pétersbourg, (1914) 405, 

‘) Preliminary experiments of this kind were begun during my stay at the 
Geophysical Laboratory in Washington, (U.S. A.), in the winter 1910-1911, 
and I wish to express my thanks here once more to my friend Dr. A. L. Day 
for his kind assistance and most valuable advice in this matter. Through these 
preliminary experiments the availability of the method up to 1200° C. was clearly 
established by me, and it became quite clear, in what directions improvements 
were necessary. The further development was hindered by the building and equip- 
ment of the new Chemical Laboratory of the University of Groningen: not earlier 
than November 1913 could the first measurements of the present series be made. 


With the increase of the temperature of observation, the experimental 
difficulties of precision-measurements increase very rapidly : measure- 
ments, which at room-temperature are of the utmost simplicity, are 
often very difficult at 400° C., and commonly almost impossible 
above 1000° C. This fact explains, why it has not been possible 
until now, to communicate the results obtained, because only an 
extended experience could prove to us the reliability of the method 
used and the degree of accuracy obtainable. 


§ 2. Of all the methods hithertho deseribed for the determination 
of surface-tensions, the one most used is the method of measuring 
the rise of the liquid in capillary tubes. Ramsay and Suipips and 
most of the investigators who have followed, have used this method. 
It can however hardly be denied, that the absolute values of x, 
obtained by different observers with the same liquids and at the 
same temperatures, show discrepancies of considerable magnitude. 
Commonly this lack of agreement is attributed rather to the unequal 
degree of chemical purity of the materials studied, than to the methods 
employed. In many of the cases, however the discrepancies were 
found with liquids, which can be obtained in a state of complete 
purity without extraordinary trouble; so that one is easily inclined 
to the belief that the method of measuring the capillary column 
includes some sources of error which are not yet sufficiently known. 
Possibly adhesion to the walls of the tubes plays a certain role in 
it, or perhaps the influence of the angle between liquid and 
solid material may be not completely negligible, as is ordinarily 
assumed. 

However there is a decisive argument against the use of the 
method of capillary ascension in the following investigations; the 
walls of the capillary tubes used, were ahvays damaged in a greater 
or less degree by the action of the molten salts. A microscopical 
examination of the walls of the tubes readily revealed this fact. 
The method cannot be employed therefore at temperatures, exceeding 
400° C., because the liquids will always be contaminated and the results 
will be almost valueless. Furthermore, the method assumes, that a rather 
long column of liquid can be held throughout its full length at a 
constant and uniform temperature. At high temperatures this condi- 
. tion can searcely be fulfilled. The study of large platinum resistance- 
furnaces has shown convincingly, that even in a central furnace- 
tube of about 26¢.m. length and 4,5 ¢.m. diameter, with the heating- 
coil wound inside, the space of really constant temperature is scarcely 


332 


longer than 4 or 5 em.') Therefore it is absolutely essential in every 
method intended for exact measurement at high temperatures, that 
the working-space be reduced to dimensions as small as possible. 
With respect to the measurements of temperature under such con- 
ditions, the available methods will permit making them with an 
accuracy of 0°,1 C.,*) which is more than sufficient for the purpose. 
On the other hand, the necessary measurements of the surface-energy 
must be made in such a way, that the results will have the same 
degree of accuracy at the highest temperatures, which they possess 
at lower temperatures, while at the same time the liquid to be 
studied must be restricted to a space of one or two cubic centimeters. 


§ 8. To fulfill these postulations, there is a method which can_ 
be used under certain conditions, which was first projected by 
M. Srvon, and later developed by Cantor, *) while it was successfully 
used afterwards for researches at lower temperatures by FrusTEt. *) 
It appeared to be possible to develop the technical procedure in 
such a way, that the method could be used, without any appreciable 
loss of accuracy, up to the highest temperatures, which can be 
measured with the platinum-platinumrhodium thermoelement. 

The principle of the method is the measurement of the maximum 
pressure HH, prevailing within a very small gas-bubble, which is 
slowly formed at the circular, knife-edge opening of a capillary tube 
immersed in the liquid perpendicular to its surface, just at the 
moment, when the gasbubble is about to burst. The sharp edge 
of the capillary tube eliminates the influence of the capillary angle. 
In this way absolute measurements of the surface-energy are possible 
in Ergs per em’., if the radius » of the tube, the specific gravity d 
of the liquid at the temperature of observation, and the depth of 
immersion 7 of the tube into the liquid, are known. To obtain the 
true value of //, the readings of the manometer require to be 
diminished by the hydrostatic pressure, corresponding to this depth 
of immersion 7. 

The method evidently can only give exact results, if the final state 
of the gasbubble represents a state of equilibrium, and is thus reached 


1) BorromLEy, Journ. of the Chem. Soc. 83. 1421. (1903) ; Lorpnz and Kaurier, 
B. d. d. Chem. Ges. 41. 3727. (1908); Trauss, ibid. 24. 3074. (1891). Vide also: 
MoryLewsk1, Z. f. anorg. Chem. 38. 410. (1903). : 

*) F. M. JAgaer, Eine Anleitung zur Ausfiihrung exakter physiko-chemischer 
Messungen bei hoheren Temperaturen. (1913). p. 36, 43. 

3) M. Smon, Ann. de Chim. et Phys. (3). 32. 5. (1851); Canror, Wied. Ann. 
47. 399. (1892). 

4) FeusTeL, Drude’s Ann. 16. 61. (1995); Forcu, ibid. 17, 744. (1905). 


Doo 


passing a series of mere equilibria; that is: the method required to 
be made practically a sfatic one, the final maximum-pressure being 
independent of the special way, in which the pressure in the growing 
gas-bubble is gradually augmented. 

Thus a very slow rise of pressure in the growing gas-bubble is 
necessary, and only in this way does it appear possible to eliminate 
the small differences of pressure in the long connecting tubes of the 
apparatus. For it is well known, that the adjustment of such small 
pressure-differences takes a considerable time, if the connecting tubes 
are relatively long. 

If the radius of the capillary tube is 7 (in em.), the specific 
gravity of the liquid d, and the observed maximum-pressure (in 
Dynes) is H, then the surface-energy x (in Erg. pro em’*.) is calculated 
from Cantor’s expression (loco cit.) : 

oh hat 


Dang am 
- 


3 


The last two terms of the second member of this equation are 
usually so small, that they can be neglected in comparison with the 
experimental errors, as being corrections of the secondary order. 

Nevertheless it has become clear, that a special correction requires 
to be applied to the values calculated in this manner, because of 
the fact, that in the theoretical deduction of this relation, a simpli- 
fication is used, which cannot be considered quite legitimate. We will 
advert to this correction lateron. (Vid.: VI; under general remarks). 

With this limitation extended experience in the use of the method 
leads to the conviction, that in the form it is used here, one ean 
obtain reliable and, within narrow limits, reproducible results. It 


has the advantage, that the surface-layer of the liquid is continually 
renewed, thus the often-observed and troublesome phenomenon of 
the alteration of this layer, need not be feared. Furthermore one 
can vary the flowing gas at will with the different liquids, to prevent 
eventual oxidations or reductions’). With these precautions the 
results can be considered as accurate at 1650° C. as at ordinary 
temperatures, if only no abnormally high viscosity is encountered 
in the liquids; for this will destroy to some extent the reliability of 
the measurements. The influence of the viscosity will be discussed 
lateron in more detail. 

Of all sources of error to be considered: inaccuracy in the 

1) As long as the gas is indifferent, i.e. as long as it does not react with the 
liquid, the results will be quite comparable, because experience teaches, that the 
differences in the values of y, measured with different gases, are vanishingly 
small in comparison with the experimental errors. 


304 


measurements of 7, of d;, of the pressure H/, of the reduction-factor 
of the observed pressure on the manometer to mercury-pressure, of 
the measurement of temperature, of the depth 7, ete., — the last 
mentioned appeared to be the most significant. If all these errors are 
assumed to be cumulative, the total effect upon the reproducibility 
of the results, even at 1650° C. is still within about 1°/, of the 
true value of x, and at lower temperatures about 0.6 °/, of that value. 
With many molten salts, where // is very great and the viscosity 
very small, the percentage error appeared to be even less than this, 
not exceeding 0,4°/,. For our purpose this degree of accuracy may be 
considered a very satisfactory one considering the enormous difficulties 
of measurements at those extreme temperatures. lt is also question- 
able, whether it will be possible to exceed this accuracy at such 
high temperatures in the near future. And if this could be 
done, it is very problematical whether much would be gained 
for the purpose proposed. For experience teaches us, that at those 
extreme temperatures all compounds are in a state of more or less 
advanced dissociation, and it can hardly be of any significance to 
express the surface-energy yx of such compounds in tenths of Ergs, 
when the uncertainty in the values of x, caused by the inevitable 
admixture of the dissociation-products, will surely be larger than 
the correction-factors following from this increase in the accuracy 
of the measurements. 


§ 4. In this and the following papers we will successively give 
an account: (1). Of the experimental arrangements and the manner 
of procedure, including some instances, illustrating the general adapta- 
bility of the method employed in different cases. (2). The results, obtained 
between .—80° and + 270° C. in the study of a great number of 
carboncompounds, in connection with their atomic constitution and the 
validity of E6érvés’ theoretical views. (3). The experiments made to 
determine the free surface-energy of molten salts, by means of the 
method here developed. In this connection we will also discuss 
more in detail the earlier attempts to solve the problem by the 
method of capillary ascension in glass-tubes. (4). Finally a discussion 
of the results obtained and a number of considerations of a more 
general kind will be given, which are suggested by the study and 
comparison of the data now available. 


§ 5. Apparatus and Experimental Equipment. 
a. In all the measurements pure, dry nitrogen, free from oxygen, 
was used, because even at the highest temperatures this gas appeared 


335 


to be quite inert, and to attack neither the compounds studied, nor 
the thermo-elements. Carbondioxyde can be used as a furnace-atmos- 
phere up to relatively high temperatures, but is often not very suit- 
able to be bubbled through molten salts under these circumstances, 
because of its character as an anhydrous acid. Furthermore, at the 
highest temperatures a_ slight dissociation is always to be feared. 
At the same time the dry nitrogen permitted us to drive out the 
air from the glass bulbs at lower temperatures, and completely 
prevented the oxidation of the organie liquids studied. 


The nitrogen employed was prepared from a mixture of pure 
sodiumnitrite and ammoniumchloride, washed by distilled water, 
and collected in a gasometer D (fig. 1). It was led through a series 
of wash-bottles ¢, filled with an alkaline solution of pyrogailol, then 
through otbers, filled with concentrated sulphuric acid (4, and finally 
through a tube /, containing a large surface of freshly sublimed 
phosphorous-pentoxide. The dried gas was preserved in a collector W, 
closed with dry mercury. When needed, it was pushed on into a 
inetal reservoir NV by means of a movable mercury-holder 7. Any 
arbitrarily chosen pressure could be used which was then read on 
the mereury-manometer A. The stopcock / carries a micrometer, 
used in the regulation of the gas-current. In the study of the organic 
liqnids, this reservoir .V was placed in the oil-thermostate (’, with 
the glass-bulbs containing the liquids tod be investigated. In this way 
the nitrogen was pro-heated to the temperature of observation, thus 
preventing disturbances of temperature in the surface-layer of the 


336 


liquid due to the small gas-bubbles emerging from the ecapil- 
lary tube. 

The regulation of the velocity of flow of the gas was obtained 
by means of the stopcock /# already mentioned, in combination with 
two accurately adjustable pinch-cocks 6, which were inserted between 
the reservoir N and the apparatus 2, carrying the capillary tube 
and its adjustments. With this arrangement no undesirable cooling 
of the surface, nor any lack of adjustment of the gas-velocity need 
be feared as a considerable source of error. 

b. The apparatus R consists of an upright rod H (fig. 2a), about 
1 meter high, and made of brass heavily plated with nickel. It rests 
on a heavy iron tripod fitted with three levelling screws. The vertical 
rod can be rotated about its axis by means of two gliding discs O 
at the foot of the pillar; they may be clamped fast when desired. 
In this way it is possible to bring the horizontal arm, bearing the 
adjusting arrangements and the movable counter-weight / into any 
desired azimuth, and to fix its position by means of the clamps at 
O and the collar at 7. With the aid of a handle provided with a 
vertical rack and pinion, this horizontal arm can be raised to any 
height and fixed there with proper clamps. This arm can also be 
moved horizontally, in order to vary its length. Moreover it appeared 
to be necessary to prevent a slight bending of the pillar A7 under 
ceriain circumstances, by means of three steel supports attached to 
H and to the iron tripod *). 

Just over #, it has at its end a rectangularly bent steel support, 
to which are attached the spiraltubes G’, made of gas-tight aluminium- 
tubes, nearly 3 millimeters wide, and also the similar tubes U, which 
however consist of much wider spirals. The latter form the continu- 
ation of the aluminiumtubes G, and their ends are firmly fastened 
to the horizontal beam, which is fixed in the laboratory just above 
the whole apparatus. The two sets of spiraltubes appeared to be 
necessary to ensure the desired mobility of the apparatus with regard 
to the manometer-connecting tubes, and also to render an effective 
operation of the adjusting devices possible. The great sensitiveness 
of the manometer makes it necessary, that all the connecting tubes 
of the instrument, as well as the spirals Gand U, should be wrapped 
with a thick layer of white flannel or asbestos, in order to avoid 
the disturbing influence of slight oscillations of temperature. 


!) In the construction of this apparatus the mechanics D. VonkK and A. VAN 
DER MB®ULEN, and the amanuensis J. J. FoukeErs, all of Groningen, have aided ina 


most practical and effective way. 


Prof. Dr. F. M. JAEGER. The Temperature-coefficients of the free Surface- 
energy of Liquids at Temperatures from —80° till 1650° C. I. Methods 
and Apparates. 


{ 
2 Poe 


mg 


Fig. 2a. 


Proceedings Royal Acad. Amsterdam. Vol XVII. 


oe 


ae 
eter 


The adjusting device FR is 
represented on a somewhat 
larger scale, in fig. 26; it is 
fixed in position over a 
resistance-furnace, and con- 
nected with the capillary 
tube made of the platinum- 
rhodium-alloy and the therro- 
element #. In this drawing 
the rectangular support with 
the spirals G are also plainly 
discernible, together with the 
hollow water-sereen ./, in 
which a current of cold water 
is continually — circulating. 
This adjusting device consists 
of two semi-circular parts 
about 40 em. in diameter. 
One part is permanently 
attached to the apparatus FR, 
the other can be fitted to it 
by means of pins and short 
tubes. The latter part has a 
circular elass- window, where 
upon the totally reflecting and 
movable (around a horizontal 
axis) prism /7 is placed. By 
means of this prism the be- 
haviour of the liquid in the 
furnace can be observed and 
controlled at every moment. At 
temperatures over 1000° C., 


coloured green glasses are 

Fig. 20, inserted in front of the prism. 

With the protection of the waterscreen / it proved possible, to use 
the manometer even at temperatures of 1650° C., without any 
disturbance from the heat-radiation of the furnace. The furnace 6 
is a platinum- (or nichrome-) resistance furnace of the usual type ’); 
it has an inside wound heating-coil, and can be heated with a 
central tube of alundum inside, up to 1400° C., and without such a 


; 1) F, M. JAEGER, Anleitung u.s.w. (1913). p. 36. 


335 


central tube, to about 1680° C. The platinum-erncible is borne upon a 
movable support of burned magnesite. which can be fixed to the 
iron support A at any elevation. 


The construction and arrangement of the part # of the adjusting 
device is elucidated more in detail in fig. 8a and 36, a giving the 


a. Fig. 3. b. 


external view from one side, / a section through it, in a plane, 
perpendicular to that of fig. 2a. 

The apparatus consists of two metal dises P, and P,, of which 
the dise P, with the tube S attached to it, can be moved horizont- 
ally round the hemi-spherical button Q, and by means of the screws 
A, and A, can be brought to any inclined position with respect to 


6: 
B09 


P,. Wf P, is turned in a horizontal direetion, the screws A, and A,, 
as well as the springs /’, and F,, (fixed at one end only) will glide 
along the upper dise P,, the whole upper part thus remaining in its 
original position. It appeared to be necessary to use a third serew 
B&B for the adjustment of the capillary tube. It is first completely 
loosened from P,, then after ?, and P, have been brought into the 
desired relative position, the screw / is turned so as to touch the 
dise P, slightly: in this way the relative position of the two plates 
is completely fixed. The tubes S and J}, (not shown in fig. 3a) are 
bent rectangularly upwards, and fitted, to the spiral tubes G. By this 
arrangement an undesirable motion of the apparatus (during the 
adjustment of the capillary tube), due to the influence of the stress and 
weight of the connecting-tubes, could be sufficienly prevented, while 
the mierometerscrew J/ at the same time remained in working 
condition. This serew J/, fitted with a drum WN and a seale D, 
serves to move the discs ?, and P, together through a known ver- 
tical distance. The serew has a pitch of 1 mm. exactly, the cireum- 
ference being divided into one hundred equal parts, it thus permits a 
vertical motion of 0,01 mm. to be measured at DY. This is more 
than sufficient, because experience proves, that no adjustment of the 
capillary tube in contact with the surface of the liquid, can be 
made with greater accuracy than about 0,1 mm. During this vertical 
motion the drum N and the micrometerscrew J/ remain in their 
original positions, because they can only move in a horizontal direction 
round the fixed part V of the apparatus. A vertical scale 7, provided 
with divisions for about 30 mm., is moved at the same time with 
the two dises P, and P,. In this way the number of revolutions of 
N can be read directly. Concerning the adjustment of the capillary 
tube with respect to the surface of the liquid, which can be made 
either visually, or with the aid of the manometer-readings, the neces- 
sary directions will be given below. 


§ 6. It was soon found, that the adjustment of the slight diffe- 
rences of pressure in the long connecting-tubes happened so slowly, 
that considerable errors in the measurements must inevitably occur. 
For this reason all the capillary tubes, with which the apparatus 
was originally equipped, were replaced by 5 mm. gas-tight tubes. 


These tubes were made in part of lead, in part of aluminium ' 


) and, 


1) Also tubes of cellon, made by the Rheinisch-Westphdlische Sprengstoffe A.G. 
in Céln a/Rh., and which may be bent in hot water, can be recommended for 
such purposes. The material is gas-tight and fire-proof; however it is difficult to 
obtain it from the plant in any desired shape. 


340 


where neeessary, were wrapped with a thick layer of asbestos. 
A considerable time had to be spent, to get all connections 
completely free from leakage ; but when this was accomplished the 
indications of the manometer were so prompt as to be practically 
instantaneous. After this no errors from this source needed to be 
feared. 

The connection of the tubes occurred in the usual way, as with 
high-pressure apparatus; these connections appeared fo remain gas- 
tight, even after a longer use. 


§ 7. For the measurement of the maximum pressures to be observed, 
originally a mercury-manometer of the type indicated by ScHEEL and 
Heusk') was used. The instrument had been modified in some details ; 
but it appeared not to be suitable for our work, because of the 
necessity of always reading tivo menisci, which was very troublesome 
with a pressure varying continually up to the moment, when the 
maximum was reached. 

This instrument therefore, which is very well adapted for static 
measurements, was only employed for the calibration of the manometer 
finally constructed. This second instrument was built on the principle 
of the manometer with two liquids. 

In the measurements of organic liquids, it was necessary to avoid 
any contamination of the connecting-tubes with the vapour of the 
manometer-liquids, so that only pure mercury could be used as one 
of the liquids in the manometer. For the second liquid we chose 
normal octane. This liquid is very thin, behaves very well in contact 
with glass-walls, and, if completely dry, appeared not to blacken 
the mercury-surface, even after long exposure. The vapourtension at 
20° C. is only 10,45 mm., the viscosity at 238° C. is 0,0052 C.G.S., 
the surface-tension at 25° C. is 21,3 Erg. pro em?*., and the expansion- 
coefficient is O0,00t18. After repeated fractional distillation, its boiling- 
point was found to be 125° C. under 758 mm. pressure, and its 
specific gravity at 25° C. was: dy = 0,6985, i.e. about 19,38 times 
less than that of mercury at the same temperature. This last relation 
operates in the following way : 

Suppose the diameter of the wider tube (fig. 4) to be D, that of the 
capillary tube d and the mercury-meniscus to the right to be @ m.m. 
higher than to the left. Then the height of the octane-column to the left 


1) ScugeL und Heuse, Ein heizbares Quecksilbermanometer fiir Drucke bis 
100 m.M.; Mitt. aus d. Phys. Techn. Reichs-Anstalt, Zeits. f. Instr. 30, (2). 45, 
(1910). 


341 


. / . at wri ] ind > 1 * 
Side (c) 1s: — m.m., 1f e = ——- — 0.0516. Suppose 4p to be the increase 
é 19,38 


of pressure (in m.m. mercury), necessaryon the right side, to sink the 


mercury-surface just 1 m.m. The mer- 
aed cury-surface on the left side, will then 
rise just 1 m.m., and the octane- 
column from ¢ to c’ (=Ahmm.), 


D 
over ; m.m. The difference of level 
ad 


of the two mercury-surfaces is now: 
(a—2) m.m., and the octane-column 


: a D : 
to the left =(-— 1+ i) mm. This 
é C 


corresponds to a mereury-column of: 


a D Dé 
—— {+ —)e={a—e+— |mm. 
& d d 


Therefore the necessary increase 


fost?) 


of pressure on the right side (= A p), 
is evidently : 


D 
(« —e+ 7°) — (a—2) m.m. = 2 + 


D 
Fig. 4. +3 Ge 1) m.m., and thus : 


€ 


or: 


Soi 


The reciprocal of the expression between }} will be seen to be 
the “multiplication factor” /’ of the instrament. With small values of 
é, (2—e) will differ little from 2; therefore it is necessary to reduce 
d ‘ _ : 
p* much as possible and to make F' as large as possible. 

In our instrument these conditions were fulfilled in the following 
way: preliminary experiment gave d = 2,406 m.m’, and D = 1257,36 
d Bee 
m.m’; thus p — 900191, and / becomes ea. 18. The reproducibility 
of the same pressure appeared to be possible within a limit of 
23 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


342 


O,1 m.m. octane, which corresponds to 0,005 m.m. mercury-pressure. 
The accuracy of the measurements was within the limits 0,05 and 
O,1°/,; it was greater than necessary in comparison with the magni- 
tude of the systematic errors of the method. 

The final form of the manometer, as it was used in all the measu- 
rements is shown in fig. 5. This final form resulted from a great 
number of experiments and numerous changes. The tube A is made 


from the best quality of hard-glass, and connects two bulbs B of 
ca. 39,9 mm. diameter with a volume of about 1380 cubie centi- 
meters ; they possess 1,2 mm. wall-thickness. The bulbs must carefully 
be chosen, and be completely cylindrical throughout their full length. 
As the height is about 110 mm., it is not easy to find tubes of the 
desired quality. The capillary tube must have an internal diameter 
of about 1,7 or 1,8 mm., and a wall-thiekness of about 2,5 mm., 
and must be suitable for precision-measurements and carefully 


TIAX “JOA ‘Wepsajsury ‘peoy [eAoy sBurpaa00.1 g 


‘9 ‘SIT 


| 
1M 


*‘sojvivddy puv spoujew ‘T “9D o0S91 II .08— wos soinjesodwmay ju 
spinbr] Jo Adsiaua-advJANGS 99IJ dy} JO S}UdIDYJa0I-2INjUJodWa_ eYL “YADAVS ‘W ‘Ad 40 J0Jd 


343 


calibrated. Its length is about 600 mm. Another tube D, of equai 
length, but about 7 mm. in diameter, serves as a connection to 
the gasapparatus. The capillary tube (bears at its top a silver 
tube EH, overlapping the tube C; it communicates with C by means 
of a silver capillary fube, and can eventually be easily removed. 
The tube C' is widened at its top-end to about 10 mm.. and con- 
nected with the silvertube in such a manner, that no dust of the 
room can contaminate the capillary tube €, while at the other end 
it communicates with a small reservoir &, partially filled with octane ; — 
this for the purpose of preventing, as far as possible, the evapora- 
tion of the liquid in C. For this reason F& is placed in the same 
thermostat as the manometer-tube. The connection of R with the 
atmosphere (or with the nitrogen) is made by means of an adjustable 
glass tube G, which opens into a very wide connecting tube leading 
to a large flask with three mouths, which is provided with dry 
caleiumoxide, with a small manometer, a tube with drying materials 
and with a connection to the nitrogen-holder. In the fig. 1 the octane- 
reservoir is indicated by C, the silver capillary tube by |S, the three- 
mouthed bottle by /. In the same way the manometer is indicated 
by w, the drying-tube by z,, and the connecting tubes by Qand H. 
The manometer is arranged in a glycerine-thermostat of the type 
usual in dilatometer-thermostats (KOunLER), however its construction 
has been varied in some particulars. The thermostats commonly sold are 
quite unsuitable for this purpose, because they commonly show leakage 
or will show it very soon; then they cannot be used for glycerine, 
which was chosen because of its refractive index and low volatility, 
because this liquid will dissolve the paste used in setting the glass- 
windows, within a short time. Two rectangular frames were there- 
fore made of brass, about 38 em. broad, and soldered to the thermo- 
stat. These frames were smoothed as perfectly as possible and 
possessed an inside furrow about 5 mm. deep and 1 em. broad, in 
which a layer of very thin rubber paste, fixed by a solution of rubber 
(in carbonbisulphide), held the two glasswindows fast. Then a second 
layer of plastic rubber was applied, and the second brass-frame was 
uniformly pressed against the former with some forty screws. The ther- 
mostat holds 22 kilos of glycerine, but even after long use it shows no 
leakage. By means of a toluene-regulator 7’ a spiral-stirrer J/ with 
motor A, and a pair of small burners 4, and 6,, the instrument is 
kept at 25°,1 C. +0°,1. Z is a thermometer, divided in 0°,1 C. 
The support # is suspended from the lid H by means of four 
movable rods /. The manometertube can then be brought into a 
vertical position by means of the screws s,, s,, s; and s,. Within 
23* 


344 


the thermostat and just behind the capillary tube C a glass-scale V 
is introduced, which possesses a very accurate division in 0,2 mm., 
by means of very fine lines (38 microns) made by the Compagnie 
Genevoise. The scale is read with a telescope and ocular-micrometer 
by the same firm, and at a distance of about 2 Meters; the enlarge- 
ment is about 25. During the readings the motor A’ must be stopped 
for a moment, because even the slight vibrations are rather annoying. 
The thermostat is wrapped with felt except for the narrow opening 
needed for the readings. Behind the manometer a ground glass-plate 
is applied, which is illuminated by two long, tube-straight-filament 
incandescent-lamps, each of 50 candle power. Between the lamps and 
the thermostat, a watertank with glasswindows, is introduced, to 
prevent heat-radiation into the thermostat. With this mode of lighting 
the fine divisions and the octane-surface are seen very distinctly, 
without any observable parallax, against an illuminated background 
and readings can be made with extreme accuracy, with the aid of 
the movable cross-hair of the micrometer. However readings of less 
than O,1 mm. appeared to be unnecessary, because of the fact, that 
the mean oscillations in the successive determinations of H, were 
about + 0,05 mm. octane, the total uncertainty therefore being about 
0,1 mm. octane-pressure, or about 0,005 m.m. mercury-pressure. 


§ 8. To bring the capillary tube into a vertical position, a mer- 
curymirror was used: by means of the screws A, and A, (fig. 3d) 
the position of the capillary tube is altered until its mirrorimage 
will seem to be in a straight line with the tube; the position of P, 
and P, is then fixed by means of the screw B. The capillary 
tube itself was origimally made from purest, iridiumfree platinum ; 
this however appeared to be too soft, and so an alloy with 10°/, or 
20°/, 


suitable capillary tubes for this purpose from the shops in trade. 


of rhodium was used afierwards. It is impossible to get any 


Therefore the rough capillary tube with its widened (ca. 6 mm.) 
upper part, was purveyed by Herarvs; the lower end was then 
carefully turned off on the lathe to a conical and sharp edge, which 
Was once more whetted on an oil-stone, if necessary. 

With some practice in this way the repairs of the damaged or 
worn capillary tubes can be accomplished within a relatively short 
time; and it proved to be possible to obtain a cross section of the 
tube, which in several directions did not deviate more than about 
0,002 m.m. from a pure circular shape, while the rim of the lower 
end measured no more than 0,01 mun. 

The cross section was determined by means of a_ horizontal 


345 


microscope, provided with a micrometer of the movable-cross-hairty pe 
with divided ‘cylinder: the diameters were measured in ten or twelve 
directions, the squares of these numbers added, the total amount 
divided by the number of measured diameters, and the square root 
from this value considered as the true value for 27. With regard 
to the measurements to be made at extreme temperatures, and on 
account of the fact, that a whetting of the capillary tubes appeared 
to be necessary almost after every set of measurements, no tubes 
with a radius of less than 0.040 ¢c.m. were used during these 
investigations. 

The platinum-rhodium-tube ends at its upperside in a carefully 
smoothed, polished brass disc; the tube of the adjustment-apparatus 
R possesses just such a smoothed circular brass-plate. As a washer 
between the two discs, a very thin ring of mica is used ; the capillary 
tube is screwed against the end of the apparatus #&, and both tubes 
are then drawn together by the aid of two steel-keys, till the discs 
are firmly pressed against each other: in this way an absolutely 
gas-tight connection is obtained. This closure appears to be a very 
perfect one, and if it is often controlled, no leakage needs to be 
feared from this source. 


§ 9. The temperature-measurements were made with our calibrated 
thermo-couples and compensator-equipment, in the way always used 
in this laboratory *). Originally it was planned to connect the platinum- 
wire of the thermocouple directly to the end of the platinum-rhodium- 
tube by means of the oxygen-flame; this tube then being considered 
as the positive end of the thus obtained thermo-couple. However 
the perfect isolation of the tube at very high temperatures appeared 
to be a serious obstacle; so the idea was abandoned, and the usual 
thermo-couples, provided with isolating Marquarpt-capillaries, was 
fixed to the platinum-rhodium-tube by means of fine platinum-wires ; 
at the other end they were connected with the ice-box J (fig. 2a). 
The wires of the element are bare over a distance of about 5 e¢.m. 
from the junction; this point lies in the same horizontal plane as the 
lower end of the capillary tube, thus being in immediate vicinity 
of its opening. Of course all platinum parts within the furnace 
(crucibles, coils, ete.) need to be made from iridiumfree platinum, 
to prevent contamination of the thermo-couples as much as possible. 


§ 10. The adjustment of the capillary tube with respect to the 


1) F. M. Jagger. Kine Anleitung u.s. w. (1913), vid. p. 16—24, 


346 


surface of the investigated liquid, can be made in the following way. 
The surface of the liquid is strongly illuminated, and now attenti- 
vely the moment is watched, when the capillary tube, while screwed 
downwards, will just make contact with its mirror-image, seen in 
the surface of the liquid. At temperatures above 500° C. ordinarily not, 
and above 1000° C. never, a special illumination of the surface is 
necessary: for the liquid radiates then sufficiently to make the obser- 
vation of the moment of contact a very accurate one. If the tem- 
perature however becomes 1400° or higher, it is often no longer 
possible to discern the end of the capillary tube from the surround- 
ings: in these cases the adjustment must be made by the aid of 
the manometer, as is further below described in some details. 

This visual method involves, even after sufficient practice an- 
uncertainty of about O.1 mm. in the case of organie liquids, which 
corresponds to ca. 0,006 to 0,008 mm. of mercury in the determi- 
nation of the maximumpressure /7. The percentage error of the obser- 
vation caused thereby, is about from 0,4 to 0,7°/,; this uncertainty 
in the adjustment of the capillary tube on the surface of the liquid, 
really appeared to be the chief source of the errors, as has been said, 
and is hardly or not to be avoided. However just at higher tempera- 
tures this and in the case of molten salts, where / is very great, the 
accuracy of the method is only slightly affected by this uncertainty. 

The other way of adjustment is this, that the capillary tube is 
approached quite near to the surface of the liquid; then carefully 
a flow of nitrogen is applied, and then, wlile the capillary tube is 
slowly lowered by means of the micrometer-screw, by observation 
of the manometer, just the moment is determined in which a sudden 
rise of pressure, caused by the contact of the tube with the surface 
of the liquid, is seey. In this way the proposed aim was also often 
attained ; but the uncertainty appeared to be here of the same order 
of magnitude, as in the case of the visual method. Furthermore it 
is necessary to ascertain that the small column of liquid, which 
often remains hanging in the capillary tube, if turned upwards, 
has no misleading influence on this observation ; first this column of 
liquid needs to be biown out by the aid of a sufficiently strong flow 
of nitrogen, before the contact with the liquid is made in the way 
just described. 


§ 11. The manometer was originally calibrated by immediate 
comparison with a mercury-manometer, which was read by means 
of a cathetometer and a divided scale. The paralaxis appeared to 
be extremely small; the accurate adjustment of the mercury-surfaces 


was highly facilitated, by putting a half transparent and diffusely 
illuminated sereen behind the manometertube, on which screen black 
lines were drawn under an inclination of about 25° with the horizon 
in such a way, that their mirror-images in the mercury-surfaces 
were visible thereupon as a bundle of very fine and easily discern- 
ible dark lines. After the application of a certain excessive pressure 
to both manometers, two observers read siimultangously both instru- 
ments; the manometers were connected with each other by a short, 
very wide tube, sufficiently protected against temperature-oscillations. 
As an example of this calibration, the following series of obser- 
vations may be reproduced here in deta‘! : 


Mercury manometer. Octane-manometer (25° C.) 
Temperature: — Observed Pressure Rise of the octane column 
pressure : 02 C m m.m. 

12,°4 7,00 6,99 124.8 
12,°6 10,23 10,21 181,8 
12,°9 12,45 12,43 220,8 
112.23 9,13 914 162,2 
12,°6 13,14 13512 235,3 
13,°0 13,78 13,75 245,0 
13,°4 12,44 122) 219,9 


A rise of the octane over 1 m.m. is therefore equivalent to an 
excessive pressure of 0,0561 + 0,0003 m.m. mercury (=74,8+0,4 
Dynes). 

After it was found, that our measurements of the free surface- 
-energy of purest water, were in so complete agreement with those ot 
VoLKMANN, Brunner, Worry, among others, we afterwards repeated 
this calibration in most cases by the accurate determination of x for 
pure water, at three or more temperatures. The factor of enlargement 
F of the manometer appeared after all to be only slowly variable : 
in Octobre 1913 e.g. it was: 17,91 in February 1914: 17,86; in 
June 1914: 18,10; ete. 


§ 12. The molten salts to be studied were in most cases placed 
into crucibles of iridium-free platinum; for the organic liquids we 
used vessels of glass of the shape indicated in fig. 7. A eylindrical 
glass tube P with rounded bottom possesses a narrower neck at 
A; a wider glass cup A is fixed round it. A tube G, closed with 
a stopper A, which is firmly fixed round the platinum capillary tube, 
possesses a collateral tube 46, which ends into a drying tube G, which 
communicates with the free atmosphere at Z, and which is filled with 


odS 


quick line. The vessel P is cleaned, care- 
fully dried, and if possible several times washed 
out with the vapours of the boiling liquid V; 


—_ 
N 


then it is filled again with a fresh quantity 
of the liquid V’, while a layer of dry mereury 
is poured into IW. The tube is placed into the 
oil thermostat, and the capillary tube with 
C the part GBC fixed to it, is lowered then, 
till G makes contact with the surface of the 
mercury. If V has reached a constant tempe- 
rature, the capillary tube is further lowered 
by screwing it so far downwards, as is necessary 


Seok 
SA 


rr ye 
ps3 


to bring it just in contact with the surface 
of the liquid. This enclosure by means of mer- 
cury insures a sufficient freedom of motion, 
while the Jiquid at the same time can be shut 
off from the air’), and the small bubbles of 
nitrogen, emerging from &, can freely escape 
at Cand Z,. All communications with the free 
atmosphere, which are present in the connect- 


ing tubes of fig. 1, are provided with drying 
apparatus, filled with dry caleium-oxide. 


§ 18. All measurements now were made in such a way, that 
always the zero-point was controlled anew accurately, before and 
immediately after each reading of the manometer. One needs to 
ascertain first, that all connecting tubes (fig. 6) are free from 
leakage, and that a diminution of the speed of gas-flow has no 
influence any longer on the value of the maximum pressure H. 
After the highest point of the octane-column is reached the liquid 
falls suddenly back to a point, which depends upon the speed of 
gas-flow, and then it begins to rise again slowly ; ete. By experience 
one learns to estimate the reliability of the measurements, by the 
particular motion of the octane in the manometer ; finally the repro- 
ducibility of the value of H needs to be considered as the decisive 
criterion for answering the question, if the real pressure of equili- 
brium in the gas-bubble has been measured. Even when the speed 
of gas-flow is varied within certain limits, this value appears to be 
reproducible quite exactly. The influence of the variation of the 
depth of immersion 7 on the manometer-readings, can be found by 


1) For if necessary, the air in the vessel P can be first substituted by a current 
of pure nitrogen. 


349 


repeated lowering of tue capillary tube over known distances by 
means of the micrometer-screw J (fig. da), and by repeating the 
readings of the manometer in every case. 

In all calculations we used the number 1383.2 Dynes as the 
equivalent of 1 m.m. mercury-pressure at 0° C.; the surface-enerey 
is expressed in Erg pro e.m.’. *) 


§ 14. As an illustration of the general availability of the method 
at all temperatures between — 80°C. and + 1650°C., we will give 
here already some few instances, relating to: water, some colloidal 
solutions, some organic liquids, and some molten salts. The specific 
weights of the organic liquids were, after a pyenometrical control 
at 25°C., calculated for other temperatures from the thermic expan- 
sion-formulae, if they were already sufficiently and accurately 
known in litterature. 

In other eases the densities at 25°; 50°, and 75° C were pycnome- 
tricaily determined, and a quadratic relation with three constants 
was calculated from these observations ; this relation was used then 
afterwards for the determination of the other specific weights. In 
the case of the molten salts the specific weights must again be 
- determined by means of a method to be described later. To use the 
numbers for the densities with more than three decimals, has no 
real significance, because the experimental errors are always of an 
order so as to make the influence of more decimals of no importance. 


§ 15. 

The curve (fig. 8) is evidently concave with respect to the tempe- 
rature-axis ; the temperature-coefficient of «is only small, and amounts 
to from 0,9 to 1,05 Erg. per 1° C. 

Furthermore in this diagram the corresponding curves are repro- 
duced for a colloidal solution of tron-oxide and for a colloidal solution 
of silicium-dioxride ; from both solutions the electrolytes were elimi- 
nated as far as possible by longer continued dialysation. 

It appears, that both curves are evidently situated somewhat above 
that for the pure solvent, although the deviations for 7 from the 
values for pure water are only very small. The temperature-coefti- 
cients are analogous to those for the solvent itself; however in the 
ease of the colloidal iron-oxyde it could be observed, that if 
such a solution was heated toa higher temperature, and if afterwards 
the determination of the surface-energy was repeated at the original 


1) The result is after all the same, as when expressed in “Dynes pro c¢.m,”. 


350 


Ie 
Water: H,0. 
0) eee ee ee 
Bo ese edad 
ea Surface: Sneeitie rie: 
HG — | | tension x in MERACe: 
| &c jin mm. mer-| . iEre. procm?,) gravity d).| Cnerey “in 
B~ Gat ere) Dynes | ea | is Erg. pro cm?., 
| PUN Ton SN ween OS Ese: 5) 2 | 
0.4 | 2.593 3457 75.8.) 11.000. |) esaae 
2 2.583 i 3444 13%) | 1.000 518.9 
| 16.4 | 2.498 3330 | 73.0 0.999 502.1 ° 
| 18.4 2.488 3317 TPAST| 0.999 500.0 
IP aay. 2.456 3275 TY 0.997 493.6 
35 2.398 | 3197 70.0 0.994 483.1 
37.8 | 2.383 | 3177 69.7 0.993 481.3 
55 | 2.291 3055 66.9 0.986 464.3 
74.2 | 2.178 | 2904 63.6 | 0.975 | 444.8 
98.5 | 2.014 2688 58.9 0.960 415.8 
99.9 | 2.004 2672 58.5 0.959 414.0 


Molecular weight: 18.02. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 


The value of x at 20° C. is thus 72.6 Erg. pro cm.?; it is more 
probable, than the often accepted value: 75.') The here mentioned 
numbers are in full agreement with those of VOLKMANN 2) (1880), 
BRUNNER 8) (1847) and Wor.ey *) (1914); they differ however consi- 
derably from the values published by Ramsay and SHIELDS 5), 


| 


lower temperature, for x a value was found, somewhat different 
from the formerly observed one with a fresh solution. Thus, although 
the iron-oxide-solution remains ‘‘stable” until relatively higher 
temperature and in general does not coagulate on heating, it seems 
however yet to undergo some zrreversible change, which is manifested 
by the somewhat changed value of the free surface-energy. 

The described method is evidently also adapted for the investigation 
of colloidal solutions of different nature; it is planned to determine 
these values so highly important for the chemistry of the colloids 
in the case of a more extended series of colloidal substances. 


1) FREUNDLICH, Kapillarchemie (1909), p. 28. 

2) VoLKMANN, Wied. Ann. 11, 177, (1880); 17, 353, (1882); 58, 633, 644, 
(1894) ; 56, 457, (1895) ; 62, 507, (1897}; 66, 194, (1898). : 

3) BRuNNER, Pogg. Ann. 70, 481, (1847). 

+4) Wor.EY, Journ. Chem. Soc. 105, 266, (1914). 

5) The other points mentioned in the diagram, have the following significance : 

W=WenperG, Z. f. phys. Chem. 10, 34, (1892); S—=Sre, Diss. Berlin, 
(1887); .R=RayweicH, Phil. Mag. (5), 30, 386, (1890); Ss = Senris, Ann. de 
VUniv. Grenoble, 9, 1, (1887); H=PRocror Hatt, Phil. Mag. (5), 36. 385, 
(1893); M—=Macin, Wied. Ann. 25, 421, (1885). These data were obtained by 
very different methods; they are evidently appreciably deviating from each other. 


351 
§ 16. Aliphatic Derwatives. 


II. 


! 


ETHYLALCOHOL: C,H;.OH. 


o : 
2} Maximum Pressure H Surface- ve, | Molecular 
gO = eee es tension 7 Specific | Surface- 
o We | rs 
eae lent saan oes ee in Erg. pro | gravity d,,| energy ” in 
S~ eae of 0° C. ae Dynes | cm?. pe pro cm?., 
— ———_ : — : : i = 
—79° 1.066 1421.2 30.6 | 0.886 | 426.2 
—24 | 0.881 1174.5 25.2 0.820 | 369.6 
0.1 0.825 | 1086.5 23.3 OF SOT = 3 345.4 
25 0.746 995.7 ZS 0.786 321.4 
35 0.724 965.2 20.6 0.777 313.1 
55 0.667 889.2 19.1 0.759 | 294.9 
74.5) 0.617 822.6 17.6 0.741 276.1 
| Molecular weight: 46.05. Radius of the capillary tube: 0.04385 em. 


Depth: 01 mm. 


The alcohol was completely anhydrous and was therefore preserved 
in a bottle with drying-tube. At the boilingpoint (78°.4 C.) the | 
value of z is 17.0 Erg. pro cm*. The mean temperature-coefficient of 
» is only: 0.94 Erg. 


Il. 


Acetic Acip: CH,. COOH. | 


: | 

= Maximum Pressure H Surface- | ei | Molecular 

s S |-— | tension x | ppecitic | Surface- 

oOo || se | . 

Sulla ate ae | in Erg. pro | gravity d,,| energy ” in 

aco cury of 0° C. | in Dynes | em?. eal Erg. pro em?. 

= | | | | 
| * ) | : | = 

26° | 0.943 | 1257.2 ON ele ate046 8) 400.7 

34.6 0.914 | 1218.5 26.1 | 1.039 390.1 

55 ORGA2 ile Sioa. eNO ed Oot 1/4 Ge aos 

70 0.787 | 1049.3 22.4 | 1.010 | 341.2 

98.5 | 0.691 | 921.3 19.7 0.987 | 304.7 


Molecular weight: 60.03. Radius of the capillar tube: 0.04385 em. 
Depth: 0.1 mm. 


| By repeated freezing and distilling, the liquid was thoroughly 
purified; its boilingpoint was 118°.1 C. The temperature-coefficient is 
between 26° and 55° C.: 1.3 and preserves that value up to the boiling- 
point. At the last temperature the value of x is: 17.7 Erg. pro cm2?. 


352 


Specific Surface-energy 
in Ergs pro c.m2, 


75 


70 


65 


60 


* Observat. of Vorkmann, and of BruNNER \ x 
© Observations of Wor.ry (1914) d 
© Observations of JancER (1913) és 


* Observat. with SiQ,-, and Fes O3esol. (1914) 


55 eee 
10° 0° 10° 20° 30° 40° 50° 60° 70 80° 90° 100° Temperature. 


Fig. 8. Surface-tensions of pure water and colloidal solutions 
at different temperatures. 


Although acetic acid doubtless is a gradually dissociating liquid, 
and in accordance with this manifests only a small temperature 
coefficient of uw, this last remains constant, contrary to the cases, 
where the curves appear to be concave or convex. 


z Maximum Pressure H Surface- Specifi | Molecular 
g° ! ——| tension z EERE Surface- 
oO . . 
Beg |e ‘ Si ike in Erg. pro gravity d,, energy » in 
s~ cury of 0° C. in Dynes em?. “| Erg pro cm?.) 
—19.9| 1.237 1649.2 35.5 1.095 985.3 
0.7} 1.167 | 1555.8 332) 1.075 941.2 
8.5 1.142 H 1523.2 32.9 1.068 928.4 
2oE2 1.077 1435.9 31.0 1.050 | 884.8 
34.5 1.044 1391.9 30.0 1.041 861.2 
50.1 0.994 1325.2 28.5 1.025 | 826.6 
69.2 0.920 1226.8 26.3 1.005 | 712.9 
102 9.804 1071.8 23.0 0.969 692.5 
124.5 0.723 963.9 20.6 0.945 | 630.7 
144 0.660 880.2 18.8 0.924 584.3 
148.7 0.649 866.4 18.5 0.919 | Silla 
171 0.571 761.6 16.2 0.896 | 513.9 
= ale Ns eee Par 
Molecular weight: 160.1. Radius of the capillar tube: 0.04385 em. | 


Depth: 0.1 mm. 


The compound boiled constantly at 1979.3 C.; at —50° C. it is 
solidified. At the boilingpoint the value of ~ is about: 13.7 Erg pro | 
em?,; the temperature-coefficient of » has as mean value: 2.52 Erg. 


§ 17. 


Aromatic Derivatives. 


V. 


BENZENE: C,H. 


= Maximum Pressure 
gO ie : 
Bo 

a6 in mm. mer- Dv 
@ |leury of 0°C.; ™ ~~ ynes 
= 

(o} 

By | ASOT) 1436.7 
9.5 1.055 | 1406.5 
25.1 0.969 le ed2O1R9 
35 0.920 1226.5 
55 0.836 1114.6 
74.6 0.757 1009.2 


th 


Molecular weight: 78.05. 


Surface- 
tension 7% in 
Erg. pro cm?. 


WNMNONMWW 
=—-WOANOO 
DwAW1W 0 


Depth: 0.1 mm. 


Although the mean value of the temperature-coefficient of » oscil- 
lates round 2.0 Erg., the dependence of » and ¢ is not a linear one: 
between 5° and 25° the coefficient is: 2.65; between 25° and 55° C.: 
2.12; and between 55° and 75°: 1.95 Erg. At the boilingpoint (80.°5), | 


e value of % is: 20.7 Erg. 


Specific 


895 
.889 
873 
862 
841 
817 


ooococoo 


Radius of the Capillar tube: 0.04385 cm. 


| gravity Ayo) 


Molecular 
Surface- 
energy in 
Erg. pro cm?. 


607.7 
596.6 
553.8 
530.3 
487.8 
451.4 


ANISOL: CH,.O, C Hs. 


| @o | | 
Es Maxi ressur 
aS | Maximum Pressure H Sirfake: Specific Molecular 
30 Near, ; ———| tension y in aon 
= jin mm. mer-| . Erg. proem2,) gravity d4o a eal 
3" joury of 0°C. | me Dec | a 1 Erg. pro em?. 
| | 1 
] = = | 
|—-21° hss Ai) WIEEER G7 4 39.3 1.029 874.8 
| 0.4 1306) | elAliad 37.3 1.010 840.6 
25 1210) ee eee OS cyl 34.6 0.987 UNS) | 
45 1137) eal lo l6eo: 32.5 0.970 15255) 7) 
74.4 12022 4 i 136225, 29.1 0.942 | 687.0 
| 90.8 O2962) ey 1282/52 27.4 0.927 653.9 
| 110 0.875 1167.3 24.9 0.907 | 602.9 
| 134.7 O65: 4) 102022 21.7 | 0.882 | 535.3 
151 0.700 |} 932.9 19.8 | 0.865 494.8 | 
| | 


| 


| Molecular weight: 108.6. Radius of the Capillar tube: 0.04352 em. 
Depth: 0.1 mm. 


The boilingpoint was constant at 151.97 C.; at —50° the substance 
crystallizes to a beautiful, hard aggregate of crystals. The tempera- 
ture-coeflicient of » increases, just as in the case of water, with | 
increasing temperature: between —21° and 45° C, itis: 1.88; between | 
45° and 90°.8 C. it is: ca. 2.14; between 91° and 151° its mean value is: 2.63. | 


VII. 


PHBNETOL: C,H;.0O.C,H;. 


| 
5 _ | Maximum Pressure H | Surface- Molecular 
re -| tension x Specitic Surface- 
© | |e : B Rec 
as iM er |} naDyhes ‘s aid se ae a's nae ‘A zs 
2 eaty of O° CC. : ike Pe) PXORC MS 
| | | 
= 21° 1.289 1718.5 36.8 1.006 902.1 
0.3) 1.213 1617.7 34.6 0.986 859.6 
25.2! 1.117 | 1489:0 31.8 0.962 803.1 
45 1 OSes el S8an3 29.5 0.943 755.0 
74.3} 0.931 | 124038 26.4 0.914 689.9 
90.6| 028715) i e lGie3 24.8 0.899 655.3 
| 110 0.813 1084.6 23.0 0.889 | 612.3 
184.7 0.734 | 979.0 20.7 0.855 565.6 
150.1 0.687 915.9 19.3 0.849 529.8 
160.5) 0.651 868.6 18.3 0.839 506.3 


Molecular weight: 122.1. Radius of the Capillar tube: 0.04352 ecm. | 
Depth: 0.1 mm. | 


The boilingpoint is constant at 168°; the substance solidifies at 
— 50° C. to an aggregate of long, colourless needles. The tempera- 
ture-coefficient of » can be considered as constant, its mean value 
being: 2.14 Erg. 


355 


VIL. 
AneTHoL: CHO. Csll,.CH:CH . CH (1.4) | 
2 ae 2 ore ee | 
= : Maximum Pressure | Surface- en | Molecular | 
€° pew red OE Jl “tension 2 Wareeees Surface- | 
Be inmm.mer-| 5 py _ in Erg pro | gravity dyo| energy 4 in| 
5 | cury of 0° C. | In yes | cm?. | Erg pro cm?,| 
hea i Int oa ail | mee: | 
"O47 1.267 | 1689.2 36.2 0.988 1021.8 
"45.5 1.188 | 1583.8 33.9 0.969 969.1 
ATByG)! 1.078 1438.4 30.7 0.944 893.0 
“94.2 1.017 1355.7 28.9 0.927 850.9 
115 0.929 1239.0 26.9 0.908 803.0 
135.1 0.865 1153.4 25.0 0.890 756.4 
160.9 0.787 1049.8 Dol 0.867 698.9 
192.8 0.689 919.1 19.8 0.838 623.6 
| 212.7 0.625 833.5 18.0 0.820 575.6 
230 0.588 783.9 16.9 0.809 ~ 544.9 


ei We see ett a inl eee PS [ee LEE a 
Molecular weight: 148.1. Radius of the Capillar tube: 0.04439 em.; 
in the with * indicated observations, the | 


radius was: 0.04352 em. 
Depth: 0.1 mm. 


The boilingpoint was constant at 230°.5 C.; the meltingpoint is: 2195 C. 
Between 25° and 75° C. the temperature-coefficient of » is about: 2.53; 
later on it becomes fairly constant: 2.25. At the boilingpoint the value 
of ~ is: 1.68 Erg pro cm’. 


IX 


GuasAcoL: CH,0.C 5H, . OH (1,2). 


oO 
5 Maximum Pressure H | : 
Es : : Surface- | Specific | Molecular 
$0 tension yin | | SEO 
| Ss inmm.mer- . Erg. proem?.| gravity dy.) Cnerey “in | 
| 5° leuy of o°¢,| i Dynes | jis | + Erg. pro em?. 
| | | 
| 26° 1.377 1°36.4 43.3 | 1.128 994.0 
45.5 1.302 1736.4 40.9 1.109 049.6 
66.5 1.224 1632.4 38.4 1.088 | 902.9 
86 1.156 1540.7 36.2 1.058 861.8 
106 1.087 | 1449.1 34.0 1.048 819.7 
|125 1.024 1365.8 32.0 1.029 780.9 
Hi4GmeeeeKOcose) SNP ri26500) | 12086 |) sl eitoos), I") "7394 
166 0.874 | 1166.0 27.2 | 0.988 682.1 
1184 0.803 1070.2 24.9 | 0.970 632.1 
206) oF 1027189, MIGRL COS TT asp 10,2253 0.948 | 574.8 
| | 


| Molecular weight: 124.06. Radius of the Capillar tube: 0.04803 cm. 
Depth: 0.1 mm. 

The substance boils under 24 mm. pressure at 1069.5 C.; the melting- 
point is 32° C. The temperature-coefficient of » is between 26° and 
| 46° C.: 217; between 146° and 206° the curve is feebly convex to 
| the f#axis and the mean value of the coefficient is therefore about: 


2.66 Erg. 


ae 


RESORCINE-MONOMETHYLETHER: C,H, (OH) . (OCHS) (1,3). 


EI é Maximum Pressure / 45 Molecular 
5 | Surface- Specific Saree 
50 a — | tension x in : 
= in mm. "| eravity d,.| energy in « 
BF mercury of | in Dynes | Erg pro cm?. era ace Erg’pro cm?, 
a 
—— - = : = 
—20° 2.622 | 3495.6 83.1 1.181 1850.1 
OTF Pee lS6S6 een ee 211 el 51.6 1.161 1161.9 
25.9] 1.462 1948.8 46.0 1.136 1051.0 
45.9) 1.380 1840.5 43.4 1.119 1001.6 
66.5) 1.318 1757.3 41.4 1.102 965.2 
86.5 1.252 1669.7 39.3 1.082 927.5 
107 1.196 1594.9 37.5 1.061 896.7 
125 1.140 1519.9 35.7 1.044 862.9 
146 1.075 1433.2 33.6 1.023 823.2 
166 1.009 1345.0 31.5 1.003 782.0 
184 0.956 1274.2 29.8 0.986 748.2 
206 0.862 1149.4 26.8 0.965 682.6 
| 


Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 


Molecular weight: 124.06. 


Under 25mm. pressure, the compound has a boilingpoint of 144°C. 

The observations over 180° C. relate to the substance already 
slightly dissociated, as was seen from the brownish colour of the 
liquid. At —79° C. it becomes glassy, without indication of crystal- 
lisation. At 0° and — 20° ©. also, the viscosity of the liquid is still 
enormous. 


XI. 


eee Maximum Pressure H | Pant 3 Molecular 
SS 2 pera | : UT Ace Specific Surface- 
oS ; | ension % in : 
a, in mm. : i a energy / in 
£2 | mercury of | in Dynes | Erg pro cm?. gravity dao Erg pro em2. 
o | = 

a OOK? 

—22° 1.520 2026.5 44.3 1.104 1107.9 

0 1.419 | 1892.3 41.3 1.084 1045.6 

25 1.325 1766.2 38.6 1.064 989.4 
45.3 1.250 1667.0 36.4 1.046 944.3 
70.5) 1.166 1554.4 33.9 1.022 893.2 
90.1 1.090 1453.2 31.7 1.004 844.6 
116 1.007 1342.7 29.2 0.980 790.6 
135.3 0.943 1257.0 27.3 0.963 TA7.9 

*162.1 0.781 1041.0 24.4 0.939 679.8 

*189.9| 0.700 932.8 21.8 0.914 618.4 

*210 0.637 849.5 19.8 0.894 570.0 


Molecular weight: 138.08. Radius of the Capillary tube: 0.04439 cm.; 
in the with * indicated observations the 
radius was: 0.04803 cm. 

Depth: 0.1 mm. 


The substance has a constant boilingpoint at 214°.5 C.; the liquid 
can be undercooled to — 76° C., and solidifies to a crystal-aggregate, 
wich melts at —52°C. At lower temperatures, as far as to 0° C., the 
temperature-coefticient of » is rather large: 2.83 Erg; later it is fairly 
constant, with the value: 2.25 Erg. 


HypRocHINON-DIMETHYLETHER: CyH, (OCH), (1, 4). 


g ; Maximum Pressure HH Surface- 
a0 tension x 
See in mm. in Erg 
g= | mercury of | in Dynes pro em. 
= 0° C. 

66° 1.106 1474.5 34.7 
86.5 1.031 1374.1 32.3 
106 0.974 1299.2 30.5 
126 0.909 1213.8 28.4 
146 0.843 1124.4 26.4 
166 0.775 1032.7 24.2 
184 0.709 945.3 22a 
206 0.628 837.0 19.5 


Specific 
gravity d 40 


1.036 
1.008 
0.990 
0.976 
0.957 
0.938 
0.921 
0.901 


Molecular 
Surface- 
energy » in 
Erg pro cm?, 


905.4 
858.3 
820.3 
dithle| 
726.2 
674.7 
623.7 
558.4 


Molecular weight: 138.08. Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 


The meltingpoint of the substance is at 56° C.; it boils under a 
pressure of 20 mm., at 109° C. On cooling first a glass is obtained, 
which gradually crystallizes in fine needles. Between 66° and 106° 
the temperature-coefficient of » is about: 2.11; between 106° and 166°, 
about: 2.46; and between 166° and 206° C., about: 2.88 Erg. The 
relating curve is therefore concave to the f-axis, 


§ 18. Heterocyche Derivatives. 


XII. 


PyRIDINE C;H,N. 


g Maximum Pressure Surface- eas Molecular 
ay tension Sa Surface- 
Oo . . . 
a, in mm. in Erg avity d,,| energy in 
BF mercury of | in Dynes in em? ch eee Erg pro cm’, 
= ONC: 
—19 1.698 2263.8 48.9 1.078 827.8 
—20.5 1.430 1906.5 41.1 1.018 722.9 
0.1 1.329 1771.8 38.1 0.998 679.0 
25 1.215 1619.8 34.9 0.975 631.8 
35 Lol 1569.2 33.8 0.962 607.3 
55 1.099 1465.2 31.5 0.942 583.4 
14 1.022 1362.5 29.3 0.923 550s 
92.5 0.960 1279.9 PACS: 0.904 523.5 


Molecular weight: 75.09. 


Depth: 0.1 mm. 


The pyridine crystallizes readily at —52° C.; thus the measurements 
at —-79° C. relate to a strongly undercooled liquid, The curve, giving 
the dependence of » and ¢ is not quite regular. At the boilingpoint 


Proceedings Royal Acad, Amsterd 


am. Vol. XVII. 


Radius of the Capillary tube: 0.04385 cm. 


358 


XIV. 


o . 
EES Maximum Pressure H Surface- BY ia Molecular 
a tension , perie Surface- 
ere inmm. | in Erg gravity Ayo energy # 
| E er re of | in Dynes pro em?. in Erg 
—70° eiey ||  Uleil - 47.4 1.036 950.8 
—20.7| 1.246 1661.5 | 39.2 0.986 812511) 
0 | 1.165 1553.2 | 36.6 0.965 7169.7 
25.8] 1.074 1432240) SB lod 0.940 721.2 
46 0.999 1332.5 31.3 0.920 679.6 
66.5) 0.928 1236.9 29.0 0.900 638.9 
86.5 0.846 1128.5 26.4 0.881 590.0 
106 OFIST 2) a s104953. 4) 24.6 0.862 557.8 
126 0.718 957.7 22.5 | 0.842 518.2 


2-PICOLINE: C;H, (CH) N. 


Molecular weight: 93.07. Radius of the Capillary tube: 0.04803. 
Depth: 0.1 mm. 


The liquid, which is boiling constantly at 1339.5 C., can be under- 
cooled as far as —74° C.; it solidifies at — 64° C. and melts there 
very rapidly. Between — 70° and — 21°, the temperature-coefficient 
is about: 2.83; afterwards the mean value remains about: 2.02 Erg. 


EV 


_CHINOLINE: CoH, - N. /3H3. 


o 

hee Maximum Pressure H L Surface- Molecular 
€° | ee MELONS LOT Specific Surface- 

| © | - 
ie baer a | in Erg. pro gravity d,.| energy » in 
a= ees of PO, in Dynes em?. = Erg. pro.cm*. 
es 

—21° 1.682 | 2242.4 49.1 | A124 | eGO RO 

0 1.608 2143.8 47.0 | 1.108 1121.1 

*24.8) 1.562 2082.5 | 44.7 | 1.089)- 9) 107826 
*45.2) 1.486 1981.1 42.5 | 1.073 | 1035.6 
*714.3 W319) 99 eel838 52 39.4 | 1.051 973.5 
*94.7 1.303 1737.1 37.2 1.034 929.1 
115 210) 3)" 61320) 9) 35.2 1.018 888.4 
135.2 1.135 | 1513.8 | 33.0 1.002 841.7 
160 1.047 | 1395.9 | 30.4 0.981 786.4 
192.5 0.929 |} 1239.0 | 26.9 0.954 708.9 
213 | 0:855, 113959 25.7 0.938 658.3 
230 0.797 ° || 1063.3 = |) 23,0 0.924 619.2 


Molecular weight: 129.07. Radius of the Capillary tube: 0.04439 em.; 
in the with * indicated observations, the 
radius was: 0.04352 em. 

Depth: 0.1 mm. 


The boilingpoint was constant at 233° C.; the liquid can be under- 
cooled as far as —50°, and then crystallizes, melting readily at —25° C, 
The temperature-coefficient of » increases with the temperature: 
between —21° and 45° C. it is: 1.92; between 45° and 115° C.: 2.10; 
between 115° and 230°: 2.33 Erg. At the boilingpoint the value of x 
is: 22.7 Erg. pro cm’. 


359 


Molecular Surface- Fig. 9. 
energy, in Erg pro c.m2. 
7790 


1160 
7730 
7100 


7070 


“80°-60°-40° -20° 0° 20° W* 60° 80° 100° 120° 140° 160° /S0° £00° 220° 240° Temperature 


24* 


Some of the curves, which relate to these organic liquids, are 
reproduced here in the usual graphical way (fig. 9); the corresponding 
critical temperatures of the liquids, so far as they are known, are 


360 


mentioned and written between () behind the names of the 
substances investigated. 
19. Salts of the Alkali-Metals. 
XVI. 
a ee 
| POTASSIUMCHLORIDE: ACl, 
lem eu eee 
= &| Maximum Pressure Surface- Molecular 
Ee ; Specitic 
ae ico} a = tension x re Surface- 
| a | {lure ° 
Be ° | in mm. mer- in Detieg fn re Pr | etevity idgo| PROTEUS 
'5 £| cury of 0°C.| J em’, Erg pro em?. 
ie ck | | 
| 799:5| 3.015 4019 | 95.8 1.509 1290.0 
| 827.1 2.957 | 3942 94.0 1.492 1275.3 
861.5 2.873 3830 91.3 1.470 1251.0 
| 885.1 2.819 3758 89.7 1.456 1237.0 
908.5) 2.768 3690 88.0 1.442 1221.3 
| 941 2.697 3595 85.8 1.421 1202.6 
| 986 2.582 3442 82.2 1.396 1165.8 
1029 2.484 3311 79.1 — = 
1054 | 2.425 3233 iliez _ os 
1087.5 2.361 3147 1522 — — 
|1103.6 2.313 3083 USsa1l — — 
11125 | Poel fe) 3033 72.5 — _ 
1167 2.182 2909 69.6 — — 
Molecular weight: 74.56. Radius of the Capillary tube: 0.04736 em. 


at 15°C. The expansion-coefficient is here 
0.0000083. 
Depth: 0.1 mm. 


The salt melts sharply at 771° C.; after four hours heating between 
900° and 1100°, it solidifies at 769°C. It evaporates rapidly at 980°, 
at 1160° with great speed. Just as in the case of the other alkali- 
salts, the vapours are doubtlessly acid, while the solidified mass gives 
an alkaline reaction, if dissolved in water. The gradual dissociation 
lowers the value of the maximum pressure more and more, as is 
seen from repeated experiments after a longer heating 1100° C. 

As some illustrations of the changes caused by the commenced 
dissociation of the salt, the following measurements are given, which 
were made after a heating at 850° and 1150° C. during full four hours: 


| At 848° C. the maximumpressure was found to be 2.821 mm, mercury 
| 904 2.720 
| ” . ” ” ” ” ” » ” S = ” ” 

” 941 ” ” ” ” ” ” ” ” 2.645 ” n 

” 956.5 » » ” ” ” ” 5 a) 2.615 ” ” 

” 1037 ” ” ” ” ” ” yn 7” 2.455 ” ” 


All values are evidently lower than the previously observed ones, 
and at the lower temperatures, at which the observations were made 
after the longest heating of the salt, the decrease is most appreciable. 


361 


XVII. 


POTASSIUMBROMIDE: (Br. | 


Temperat. Maximum Pressure / Surface- 
LTC Cys | aueeenntan | ennennmnnann LENS LONI air 
in mm. 
(corr.) mercury of | in Dynes | Erg. pro cm?. 
0° C. 
° 
775 2.102 3602 85.7 
798 2.642 3522 83.8 
826 2.585 3446 82.0 
859 2.504 | 3338 79.5 
886.5 2.450 | 3266 71.8 
920 2.376 3167 75.4 


Molecular weight 119.02. 
Radius of the Capillary tube : 0.04728 cm. at 15°C. 
Depth: 0.1 mm. 


The dissociation and splitting off of hydrogen- 
bromide and bromine is observed at 825° C. At 
940° C. the evaporisation and dissociation of the 
salt have become so rapid, that measurements | 
at higher temperatures seemed to be without 
any real significance. 


XVIII. 


POTASSIUM IODIDE: AV. 


Temperat. Maximum Pressure H Surface- 
mya Ce tension x 
(corr. on in mm. in Erg 
G. Th.) mercury of | in Dynes pro cm?, 

0° C. 
Sie ane meta nar a. 
737 2.372 3162 15.2 
164 2.274 3031 72.1 
866 2.106 2807 66.8 
873 2.097 2795 66.5 


Molecular weight: 165.96. 
Radius of the Capillary tube: 0.04728 cm. at 15°C. 
Depth: 0.1—0.2 mm. 


The salt melts at ca. 700° C. Already at 750° C. 
it evaporates rather rapidly, and at 900° C. with 
dissociation into hydrogen-iodide and iodine. Meas- 
urements at higher temperatures can have hardly 
any significance. 


812 2.183 2910 69.2 


362 


XIX. 

SoprumcuLoripn: NaCl. 
o a 
= E Maximum Pressure H Surface- bas me Molecular 
gOS st ANS tension haa Surface- 
o° : ; 
Be |; Ula in Erg. pro gravity d energy ” in 
ens aeee OG in Dynes em? 4 Erg. pro em?. 
Bias E 
802.6 3.580 4772 113.8 1.554 1275.9 
810.5 3.572 4762 113.5 1.549 1275.4 
820.8 | 3.552 4735 112.9 1.543 1270.8 
832 3.520 4692 111.9 any 1262.6 
859 | 3.457 4608 109.9 1.523 1247.7 
883.2 | 3.401 4534 | 108.2 — — 
907.5 3.345 4459 | 106.4 — 
930.6 3.285 4379 104.5 — — 
960.5 3.227 4302 102.7 — 
995.5 3.132 4175 99.7 — _ 
1037 3.047 4062 97.0 —- — 
1080 2.951 3934 94.0 — — 
1122.3 2.864 3818 91.3 -— — 
1171.8 2.761 3681 88.0 — = 


Moleculair weight: 58.46. Radius of the Capillary tube: 0.04736 cm. 
15°RC 


Depth: 0.1 mm. 


at 
{ 


The pure salt melts at 801° C. At 1080° it evaporates already rapidly, 


at 1150°C. very rapidly. 


The temperature-coefficient of « calculated in 


the few cases, where values of specific gravity were available, is very 


small: 


strong alkaline reaction; 


about 0.57 Erg. The solidified mass gives in water a rather 


reaction. 


the vapours of the heated salt have an acid 


SODIUMSULPHATE: Na,SO,. 


2 a ‘ 55 

2 SI Maximum Pressure H Saitate: 

oe oS = : 

Ey ° g tension yin 

BS g |inmm mer | in Dynes | Bre procm 

= 3 
900 6.285 8379 194.8 
945 6.247 8328 189.3 
990 6.209 8278 188.2 
1032 6.149 8197 186.5 
1077 6.088 8116 184.7 


Molecular weight: 142.07. 
Radius of the Capillary tube: 0.04512 em. 
Depth: 0.1 mm. 


The pure salt melts at 884° C. If heated 
to 1100° C. the solidified mass! gives in water 
a rather strong alkaline reaction, indicating 
a dissociation. Measurements at higher tempera- 
tures than 1100° C. thus seemed to be useless. 


XXI. 
SopDIUMMOLYBDATE: Na,Mo0,. 
| 
Oo : 
Bos Maximum Pressure H Satraee: 
ra E | tension x in 
S2)inmm.mer-| . i 2 
5 cury of 0°C, | ™ Dyueaia pe rere eee 
| eeu rie i 
698.5 6.091 8122 214.0 
| 728.5} 5.975 7967 | 210.0 
Tl 5.921 7893 208.1 
777 5.828 7770 204.9 
| 818.8 5.757 7675 | 202.4 
| 858.5 5.657 1542 199.0 
; 903.8 5002 7401 | 195.4. | 
| 948 5.436 7247 191.4 
989.5 5.330 7106 187.7 
1035 5.224 6966 184.1 
1078.5) 5.141 6854 | 181.2 
/1121.5 5.070 6760 178.8 
1171.5 4.998 | 6654 176.1 
1212 4.947 6595 174.6 
= 
Molecular weight: 206. 
Radius of the Capillary tube: | 
0.05240 cm. 
Depth: 0.1 mm. 
The compound melts at 687° C. to a | 
_colourless liquid. = 


XXII 


| LITHIUMSULPHATE: Li,SO,. 


\o 
5 Maximum Pressure // Surface- 
a H tension , 
|@29 6 ; . 
}259} in mm. in Erg 
a= mercury of | in Dynes pro em2, 
a 0° C. 
860° 6.361 8481 223.8 
873.5 6.342 8455 223.1 
897 6.303 8403 221.8 
923 6.256 8341 220.2 
962.5) 6°169 8224 217.4 
| 976.8) 6.146 8194 216.4 
|1001.2 6.099 8132 214.8 
1038.5 6.027 8035 212.3 
| 1057 5.987 7982 211.0 
|1074 5.953 71936 209.8 
|1089.5 5.923 7897 208.8 
1112 5.879 7838 207.3 
1156.5 5.791 77120 204.2 
1167.5 5.766 71687 203.4 
1183.5 5.737 7649 202.4 
1192.2 5.718 71624 201.8 
1214 5.675 7566 200.3 
Molecular weight: 109.94. 
Radius of the Capillary tube: 
0.05240 em. at 16° C, 
Depth: 0.1 mm. 
The salt was prepared frompurest lithium- 
carbonate and sulfuric acid, carefully dried 
, and heated at 900° C.; it melts at 849° C. 
After being heated to 1200° C., the substance, 
shows an alkaline reaction with water. Also 
here it is of little significance, to pursue the 
measurements to higher temperatures. 


XXII. 


LITHIUMMETASILICATE: Li,SiO;. 


5 : = Maximum Pressure 7 Surface- 

EOS ee eS tension 

oo | a . 

a. 8 in mm. in Erg 

8 sues mercury of | in Dynes pro em2. 

a 2 O°RC: 

al SSS SS Ee = SSS ee —_ 

1254° 11.82 15759 374.6 
1380 11.29 15052 358.2 
1421 Lee 14958 356.2 
1479 11.11 14812 352.8 
1550 10.97 14626 348.7 
1601 10.90 14532 346.6 


Molecular weight: 90.01. 
Radius of the Capillary tube: 0.04706 cm. 
Depth: 0.1—0,.2 mm. 


The analysed metasilicate was perfectly pure. It 
melts at 1201°C. The temperature-coefticient of » is 
very small. 


365 


§ 20. In the case of Porassiumcunorate: ACUO,, the maximum 
pressure HH was 3,573 mm. mercury at 413°.5 C; at 448°.5 C. 
it was: 3,540 mm. The radius of the here used silver-capillary tube 
being: — 0.03460 em., the free surface-energy is calculated : 

At 413°.5 C. 7% = 82,4 Erg. pro cm’. 
At 443°.5 C. ¥ = 8156 Erp. proven: 

At the last mentioned temperature the salt commenced to decompose 
already distinctly, while O, was split off; at higher temperatures 
therefore the values of y appeared to increase gradually by the 
generation of AC/O, and KC7. 

It was not possible therefore to investigate the values of the 
temperature-coéfficients at higher temperatures; in every case however 
they seem to be rather small. 

With Stnvernirrate: AgNO,, the value of x is about 164 Erg. 
pro em*. at 280°C; at 410°C. it is about 153.8 Erg. In this case 
the temperature-coefficient is also in the neighbourhood of 0.6 or 0.9, 
— this being a rather small value too. 


§ 21. It is not my intention, to discuss now already the here 
mentioned data, nor to add the remarks, which are suggested thereby. 
It is better to postpone that task, until the complete experimental 
material now available will be published. The given instances may 
however prove, that the question: how to measure the surface-tensions 
of liquids with great accuracy within a temperature-interval, from 
— 80° C. to 1650° C., may be considered now as completely solved. 


Groningen, May 1914. Laboratory of Inorganic Chemistry 
of the University. 


Chemistry. — “The Temperature-coefficients of the free Surface- 
energy of Liquids, at Temperatures from —80° to 1650° C”. 
II. Measurements of Some Aliphatic Derivatives. By Prof. 
Dr. F. M. Jagger and M. J. Suir. (Communicated by Prof. 
P. v. Rompuren). 


§ 1. In what follows the data are reviewed, which were obtained 
by us in the study of a series of aliphatic derivatives after the 
method formerly described by one of us‘). 

With respect to the liquids here used, we can make the following 
general remarks. No product of commerce, not even the purest ob- 


366 


tainable, can be esteemed suitable for this kind of measurements: the 
small traces of humidity already, which even the best chemicals always 
contain, are sufficient to make the results unreliable. Most of the orga- 
nical liquids of commerce however seem to contain several admixtures, 
in small quantities or even larger quantities of water. We often 
obtained a first purification by distilling a small fraction from it, 
whose boiling point remained constant between 1° or 2° C. In 
several cases even this appeared not to be possible: in such case the 
preparation was dried during some days by means of anhydrous 
sodiumsulphate; then, if the special character of the substance did 
not forbid this, it was dried again during a long time by means 
of freshly sublimed phospherpentoxide, after which the fractional 
distillation was tried again. Commonly it appeared to be possible, ’ 
to separate from it a fraction, whose boiling point remained constant 
between 1° or 2° C. With some preparations we succeeded in drying 
them by means of metallic sodium. After very dry fractions, boiling 
within a few degrees, had been obtained in this way, they were once 
more distilled with a small flame only, or on the water-bath, under 
atmospheric or reduced (12—20 mm.) pressure; in this operation 
only the fraction, boiling within an interval of 1 C°., was used 
for further treatment. The liquid was then cooled during several 
hours in a closed vessel, by means of a mixture of salt and ice, 
or by a bath of, solid carbondioxide and alcohol. If it erystal- 
lized, a further purification was often possible by repeated 
freezing and decanting. Often a very thin layer of a solid substance 
(eventually of ice) was deposed at the walls of the vessel, the rest 
remaining liquid and transparent; the liquid portion was poured 
into a dry, clean vessel then, and the said operation repeated, 
till no solid layer any more appeared. [f however the phenomenon 
continued to appear, the liquid was treated again at least during a 
week with fresh phosphorpentoxide, and the freezing repeated again 
and again. Finally the purified liquid was distilled once more under 
atmospheric or reduced pressure; only the fraction, boiling within 
half a degree was collected then for the measurements. It is hardly 
necessary to mention, that hygroscopical liquids were preserved and 
treated in a suitable manner. The thus obtained liquid was commonly 
only a jvery small fraction (10°/, or 20°/,) of the original commer- 
cial preparation; it must be remarked, that the observed boiling- 
temperatures often differed appreciably from the data, given in the 
literature, and in several cases appeared to be dower than those; 
— which perhaps can be explained by the fact, that in the distil- 
lations, described in the literature, the liquid was heated éoo rapidly. 


In our experiments the speed of distillation often did not exceed 
about six drops every minute. In some cases, e.g. with ¢olwene, it 
was impossible to distil from the product of commerce a fraction, 
fulfilling all conditions; in such cases the substance was prepared 
in some other way, e.g. the mentioned toluene by dry distillation 
of purified calciumphenylacetate; ete. In the series of compounds 
described, several were taken from the collection of scientific prepa- 
rations of this laboratory; from these also only the small, constantly 
boiling fraction was used for our purpose. 

§ 2. Notwithstanding the by no means negligible differences of 
the boilingpoints observed, the specific gravities of the liquids in 
most cases differed only slightly or not at all from the data, given 


in the literature. If this was the case, — and we always controlled 
this by some pycnometrical determinations at 25° C., — the specific 


gravities at other temperatures were calculated from the expansion- 
formulae eventually already determined. If the direct determination 
of d=’ did not agree with the number, given in literature, or if the 
expansion-formula was not known accurately enough, three specific 
gravities, e.g. at 25°, 50°, and 75° C. or at a higher temperature, 
were determined pycnometrically, and from these determinations an 
empirical equation of the second degree with respect to ¢, was calcu- 
lated. This is completely sufficient here, because the specific gravities 
were all abbreviated with three decimals: an account of the densities 
in more than three decimals, must be esteemed valueless here, with 
respect to the obtained accuracy of the measurements. With most 
liquids, the mean decrease of the specific weight for 1° C. does not 
differ largely from 0,001. For temperatures of — 70° and above 
100° C. it was often necessary to extrapolate by the aid of the 
established empirical formulae ; although conscious of the uncertainties, 
which are always connected with such extrapolations, we are of 
opinion that we have not introduced here in this way errors of appre- 
ciable amount, because for these values such an error could manifest 
itself only in the third decimal place, and dilatation of the liquids 
occurs ordinarily in so regular a way, that the probability of heavy 
errors is thus highly diminished by this circumstance. 

Moreover another way was not available at this moment, if not 
with large sacrifice of time and labour. 


§ 3. In the following the obtained results are collected in tables. 
For the value of 1mm. mercury at 0°C., 1333,2 Dynes (45°), was 
ealeulated, and this value was used in all further calculations; in the 
tables all numbers for x and u are adjusted by the necessary corrections. 


368 


The graphical diagrams relate to the variation of the so-called 
“molecular” surface-energy mu with the temperature; in the same 
diagram analogous, homologous compounds or such, related by simple 
substitutions, are put together; this will be of practical use for the 
comparative considerations later to be given, and allows a rapid 
review of the behaviour. For the construction of the diagrams, not 
the numbers of the tables, but those following directly from Cantor’s 
formula, are used; therefore the correction, necessary to derive the 
absolute value of 4 from these readings by diminution, are indicated 
on each curve in the diagrams. 

§ 4. Aliphatic Derivatives. 

This series of measurements relates to the following aliphatic 


Molecular Surface 
Energy in Erg. pro cm?*, 


7000 
« 
990 = 
~ 
940 x, 
‘ 
9/0 os 
Ne 
SSO \ 
\\ 
\ 
G50 NS 
‘ 
20 as 
2 . 
e 
790 Saw 
eR 
ak 
760 Ss 
=2. 
730 NG = 
‘ ° 
700 YE 
« 
670 ee 
XN 
640 4 x 
. « 
610} , \ 
x . 
bs \ 
I8O x Xe a. 
. 
5501. NS se 
xy Xe NS \ 
5200, SO 
RK Pee? 
490 Hs eee 
Sues co 
ease Te Cp 
460 AS: SS SoS “SOSo 
See Sa ORS é 
430 b. aS Stee SS “3556 
Ss era! Ss, as Co. . ne 
~ aa ’ 5 , 
400 SS a ne =< 
; ne 2 eee 
5 ASS SNS 
370 ee 2) Sc atid 
340 Se Se 
[OSs SA -8 
JII0 EE ote 
(ae. SB 
280 SLPS, =a 
250 


“50° -60°-40° -20° O° 20° 40° 60° 80° 00° 120° 740° 160° 780° 200° 220°247° Temperature 


Fig. 1, 


369 


substances: norm. Propylalcohol; Isobutylalcohol; Diethylether ; Ethyl- 
formiate; Ethylchloroformiate; Ethylacetate, Methyl-, Ethyl-, and 


norm. Propyl-alcohol: C3H;. OH. 


= Maximum Pressure Surface- Specifi Molecular 
aS tension pecie Surface- 
Es in mm. mer-) _ in Erg. per gravityd,, | energy v in 
Bie cury of in Dynes: cm’. 4° | Erg. pro cm?, 
& OOK: 
~76 1.170 1559.8 33.4 0.881 557.4 
—21 0.924 1245.4 © 26.6 0.837 459.3 
0 0.875 1167.3 24.9 0.820 435.9 
25.5 0.807 1075.4 22.9 0.800 407.5 
45 0.755 1006.4 21.4 0.784 386.0 
74.5 0.679 905.3 19.2 0.759 353.9 
90.6 0.638 850.2 18.0 0.746 335.6 
| 
| Molecular weight: 60.06. Radius of the Capillary tube : 0.04352 cm. 
Depth: : 0.1 mm. 
The substance boils at 96°.7 C. constantly. 


Isobutyl-alcohol: (CH3). CH .CH,OH. 


v . 
a Maximum Pressure Surface ee Molecular 
so tension x Beeme Surface- 
a” jin mm. mer- in Erg. pro ravity d,,| energy » in 
EE | cury of in Dynes 2 Seat aes 2 
2 he. y; cm’. Erg. pro cm’. 
—11.5 1.149 1531.8 33.0 0.885 631.5 
—12 0.890 1186.5 25.5 0.828 510.1 
0.3 0.853 1137.2 24.4 0.817 492.5 | 
10.4 0.825 1099.9 23.6 0.807 483.9 | 
25.1 0.783 1044.5 22.4 0.794 | 460 9 
35.1 0.756 1008.0 21.6 0.785 447.7 
49.7 0.723 963.9 20.6 0.771 432.2 
69.6 0.670 893.8 19.1 0.753 407.0 
101 0.594 791.9 16.9 0.731 367.4 


Molecular weight: 74,08. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 


The compound boils at 106°.8 C. constantly; at the boilingpoint y 
has the value: ca. 16.5 Erg. pro cm’. 


370 


Tsobutyl-Isobutyrates; Acetone; Methylpropylcetone; Ethyl-Acetyloacetates 
Methyl-Methylacetyloacetate; thyl-Propylacetyloacetate; Methyl-, Ethyl-,. 


Diethylether: (CjH5)o O. 


ql Maximum Pressure 7 Surface- 2 Molecular 
SOP MAL. Be Et oes tension Specific Surface- 
ao in mm. | inErg. pro | gravity d,. | energy in 
ES mercury of in Dynes cm?. 4 Erg. pro cm? 
| 0° C. 
I-75" 0.990 1319.9 28.5 0.818 574.7 
—20.5 0.748 997.2 21.5 0.758 456.2 
0.2 0.670 893.8 19.2 0.735 415.8 
10.9 0.628 837.2 17.9 0.723 392.0 
2523 0.584 718.6 16.7 0.707 371.2 
29.5 0.574 766.2 16.4 0.703 365.9 


Molecular weight: 74.08. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 


The substance boils at 34.98 C. constantly; at the boilingpoint x is: 
15.9 Erg. pro cm? 


IV. 


Acetone: CH;.CO.CH3. 


iS Maximum Pressure 1 Surface- . Molecular 
eS u a tension x Specific Surface- 
2.0 in mm. in Erg. pro ity d energy » in 
§-= | mercury of | in Dynes | . cm2, agree es Erg. pro cm”. 
be OoRE 
EY, le oles 1647.8 35.6 0.917 565.5 
—19.5 0.971 1295.6 27.9 0.845 468.0 
Oe) 0.886 1181.3 25.4 0.818 435.4 
11.4} 0.838 1117.4 24.0 0.803 416.5 
25.5 0.786 1047.9 22.5 0.785 396.4 
35 0.740 085.6 Ake 0.772 375.9 
50.1 0.695 926.6 19.8 0.757 357.4 


Molecular weight: 58.05. Radius of the Capillar tube: 0.04385 cm. 
Depth: 0.1 mm, 


The boiliagpoint is 56° C.; the value of y is there: 19.4 Erg. 
pro cm*. 


Eye! 


Propyl-, Butyl-, Tsobutyl-, and Amyl-Cyanoacetates; Tri-, and Tetra- 
chloro-methane; and Isobutylbromide. 


V. 
— 
Methylpropylcetone: CH3.CO.C,H;. 
= 
E ; Maximum Pressure | Surface- . Molecular 
ey tension ~ Specific | Surface- 
a. in mm. | in Erg. pro ity d,. | energy » in 
5 P gravity 
s* menu of | in Dynes | em2, | 4° Erg. pro ae 
74-2 1.240 1653=2)00 35.4 | 0.936 721.4 
—20.5, 0.996 el 32729 28.3 | 0.872 604.6 
0.3) 0.913 1217.8 26.0 | 0.852 564.1 
25.5} 0.831 1107.6 | 23.6 0.826 22 
45 0.762 1015.7 21.6 0.806 486.3 
74.3 0.672 896.1 19.0 0.777 438.3 
90.8 0.613 818.1 | URS 0.761 404.7 
99.6 0.589 785.8 | 16.6 0.753 391.1 
| | 
Molecular weight: 86.1. Radius of the Capillary tube: 0.04352 cm. 
Depth: 0.1 mm. 
The substance boils at 101.93 C. constantly. 
= =| 
VI. 
Ethylformiate: HCO. O(C2H;). 
v . 
Ele Maximum Pressure H | Surface- acan Molecular 
hes tension % peeitic Surface- 
on in mm. : > in Erg. pro | gravity do energy » in 
‘= | mercury o in Dynes em?. Erg. pro cm2. 
2 ee | ee 
1605) 12289 1661.2 | 37.8 1.032 502.7 
*—16.2 0.945 1259.9 28.5 0.958 398.3 
baer aad 0.864 1151.9 26.0 0.938 368.5 
24.9 0.802 | 1069.2 22.9 0.910 331.2 
Sone 0.757 1009.6 21.9 0.899 319.3 
49.2 | 0.718 957.2 | 20.5 0.879 303.4 
be a 
Molecular weight: 50.0.5 Radius of the Capillary tube: 0.04408 cm.; 


in the observations, indicated by *, this 
radius was; R=0,04638 cm. 
Depth: 0.1 mm. 


After carefully drying, this ether boils at 54.93 C. constantly ; it 
remains a relatively thin liquid as far as —79° C. At the boiling- 
point , is 19.9 Erg. pro cm®*. 


372 


Molecular Surface- 
ee ; Bs 
Energy in Erg pro em?. Fig. 2. 


80°-60°-40°-20° O° 20° 40° 60° 80° 700° 120° 740° 760°780° 200°22G° Temperature 


VII. 
Ethylchloroformiate: C/.CO.O(C:Hs). 
vo ° 
iB , Maximum Pressure H | Surface Bane Molecular 
See —EE -| tension pectic Surface 
Be in mm. mer-) in Erg. pro | gravity d,,| energy win 
ce cay ao in Dynes em? Erg. pro cm’. 
— 15.5 1.353 1803.8 42.4 1.278 819.0 
- 21 1.046 1395.0 32.6 1.186 661.9 
0) 0.951 1269.2 29.6 1.160 609.9 
25 0.847 1129.2 26.2 1.127 550.3 
45.3 0.774 1031.8 23.9 1.095 Sila 
70.2 0.692 922.6 Dili, 1.050 466.8 
84.8 0.643 857.8 19.8 1.022 443.9 


Molecular weight: 108.49. Radius of the Capillary tube: 0.04803 cm. | 
Depth: 0.1 mm. | 


The compound boils at 91.°5 C. constantly; at this temperature x 
is 19.3 Erg. pro cm’. 


VIII. 
: Ethylacetate : CH,.CO.O(C)Hs). 
rs ] 
5 : Maximum Pressure 1 Surface- Specifi Molecular 
e- tension z Beciuc Surface- 
a. jin mm. mer-) | in Erg. pro | gravity d,.| energy # in | 
a” ony ee | in Dynes cm?. Erg. pro cm’,) 
| 
S714 | 1.274 || “1698.5 36.6 1,016 716.8 
—20 0.994 1325.2 28.4 | 0,949 582.1 
0 0.892 1189.2 25.5 0,924 532.1 
25.5 0.780 1039.9 22.2 | 0.893 473.8 
34.7 0.744 992.5 21.2 0.881 | 456.6 
55 0.679 897.2 19.1 0.856 419.3 
70 0.623 838.5 17.8 0.829 399.2 
Molecular weight: 88.06. Radius of the Capillary tube: 0.04385 em. 
Depth: 0.1 mrh. 
After very carefully drying and repeated distillation, this ether boils 
at 77.°1 C. constantly. It remains a thin liquid as far as —80° C. At 
the boilingpoint the value of z is: 17.2 Erg. pro cm’. 


25 
Proceedings Royal Acad. Amsterdam. Vol. XVII, 


IX. 
| ; | 
Methyl-Isobutyrate: (CH3), CH .CO.0O(CH5). 
o | : 
ae Maximum Pressure Surface- i Molecular 
so ie ee A BA ene Specific Surface- 
Bie | in mm. mer- | _ inErg. pro | gravity d,, | energy in 
| §- cury of in Dynes em2, 4° Erg. pro cm?, 
|e ONG: 
73° | M.296 1728.0 37.1 0.995 813.1 
21.5) 1.006 1341.9 28.7 0.936 655.1 
0.5 0.903 1204.0 syotl 0.911 597.3 
| 25.3) 0.805 1073.2 22.8 0.882 541.5 
| 45 0.727 969.7 20.6 0.859 497.9 
| 74.7 0.631 840.9 17.8 0.825 442.0 
| 91.3) 0.589 785.8 16.6 0.806 418.6 


Molecular weight: 102.08. 


The substance boils constantly at 91°.8 C. 


Radius of the Capillary tube: 0.04352 cm. 


Depth: 0.1 mm. 


X. 


Ethyl-Isobutyrate: (CH3). CH.CO.O(C,Hs). 


bol POs 


eS) 
ENE NS 


Maximum Pressure Surface- : Molecular 
ese ae we | tension x Specific Surface- 
| in mm. mer- | in Erg. pro gravity Ayo energy » in 
cury of in Dynes em?2, Erg. pro cm’, 
a ay je —— —— — = = — 
| 1.165 155352 i 33.3 0.976 805.4 
0.940 1253.2 26.8 0.913 677.7 
0.867 1155.9 24.6 0.891 632.3 
0.779 1038.6 | 22.1 0.859 582.0 
0.717 955.9 20.3 0.837 544.0 
0.624 831.8 17.6 0.809 482.4 
0.572 762.9 16.1 0.791 448.0 
0.507 675.5 14.2 0.769 412.6 


Molecular weight: 116.1. 


Radius of the Capillary tube: 0.04352 cm. 


Depth: 0.1 mm. 


The substance boils at 110.°2 C. constantly. At —76 C. it is again 
a thin liquid; it was only slightly turbid, probably by extremely fine 


crys 


tals. 


375 


XL. 


Isobutyl-Isobutyrate: (CH3),CH.CO.O(CH) .(CH . (CH3),). 


g ‘ Maximum Pressure Surface- +f Molecular 
e* — tension x SUE Surface- 
a. jin mm, mer-) in Erg. pro | gravity d energy in | 
~ cary ot | in Dynes cm. =| 4° | Erg. pro cm’. 
~16.5 1.182 1576.3 33.8 0.951 960.6 
—21.3 0.927 1236.2 26.4 0.896 780.8 
0 0.865 1S Sota 24.6 0.875 739.2 
25.4 0.785 1047.8 | 22.3 0.850 683.1 
45 0.731 974.3 20.7 0.830 644.2 
74.7 0.638 850.2 18.0 0.801 573.6 
91.1 0.596 795.0 16.8 0.784 543.1 
109.2 0.545 726.1 15.3 0.766 502.3 
134.5) 0.469 625.0 13.1 0.740 440.1 


Molecular weight: 144.11. Radius of the Capillary tube: 0.04352 cm. 


Depth : 0.1 mm. 


The compound boils at 147.°2 C. constantly. 


XIL. 
Ethyl-Acetyloacetate: CH,;CO.CH,.CO.0O(C,Hs), 
& Maximum Pressure H Surface- | S if Molecular 
ES tension x | “Pectlic Surface- 
te ‘in tim. mers) in Erg, pro | gravity dy. energy ” in 
ce cary ct | in Dynes cm. | Et'g. pro cm’, 
== = a — oa se SSS 
—20°| 1.210 1612.8 3am) e070 900.7 
1 1.133 1510.5 34.3 1.048 853.5 
S25 ea ere Lets 1483.6 32.0 | 1.023 809.2 
yaks) 1.069 1424.7 30.7 1.013 781.4 
* 49.5, 1.024 | 1365.8 29.4 0.999 155.3 
71 0.906 ae 201: Aten | 27.3 0.976 712.3 
89 0.841 1121.2 25.3 0.958 668.4 
e125 0.774 1031.9 211 0.923 587.7 
MoS 0.675 900.2 18.9 0.896 522.1 
=S1765") (05596 794.9 16.6 0.869 468.0 
| =e Pale all 4 
Molecular weight: 130.08. Radius of the Capillary tube: 0.04638 cm.; 
in the observations indicated by *, it was 
0.04408 cm.; in those by **: 0.04352 cm. 


Depth: 0.1 mm. 


The substance boils at 179.°6 C. constantly. 


25* 


Molecular Surface- 
energy in Erg pro cm2. 


720) 

690 . § 

660 y Sete 
eS 


Tempe- 


-80°-60°-40° 20° O° 20° 40° 60° 80° 100° 120° 740° 160° 180° 200° 220° 240° 260" ature. 


Molecular Surface- 
energy in Erg pro cm’ 


7020 


Fig. 4. 


“80° -60°-40" -20° O° 20° 40° 60° 80° 100°120°740' 00180200 


Temperature 


377 


XII 
Methyl-Acetylomethylacetate: CH;CO.CH(CH3).CO. 0(CHs3). 
a : Maximum Pressure | Surface- ie | Molecular 
| Sie eee | tension x | Specific Surface- 
are in mm. mer-| | | in Erg. pro | gravity d,,| energy “in 
bi ue in Dynes | cm?, as pro cm’, 
<1 | 1.477 | 1969.6 | 46.5 1.121 | 1106.2 
—21 1.218 | 1623.8 | 38.3 1.071 939.3 
0 1.137 1515s ees Bball 1.050 887.2 
20e3 1.046 1395.0 32.8 1.024 828.9 
45.5 0.985 1313.2 30.8 1.003 789.2 
710.2 0.901 1201.2 28.1 0.977 | 732.7 
85.2 0.856 1141.2 26.7 0.962 703.4 
Lees OS 68 1024.4 23.9 | 0.930 | 644.0 
138.2} 0.709 945.2 22.0 0.908 602.3 
156 0.658 877.2 20.4 0.890 566.0 
Molecular weight: 130.08. Radius of the Capillary tube: 0.04803 cm. 
Depth :0.1 mm. 
Under a pressure of 18 mm., the substance boils at 75.95 C.; in the 
at —71°C. very viscous liquid, the growing of the gas-bubbles took 
more than 60 seconds. The specific gravity at 25° C. is: Ayo = 1.0247; 
at 50°C.: 0.9991; at 75° C.: 0.9732. At © C.: Ayo= 1.0500—0,001006¢ 


—0.00000024 #. 
XIV. 


Ethyl-Propylacetyloacetate : CH3CO.CH(C3H;)CO . O(C)Hs). 


£ _ | Maximum Pressure H Sine | ato | Moteeular 
eo tension x Recinie | Surface- 
o - F y | ‘ 
Qa. jin mm. mer-| _ in Erg. pro | gravity d,,| energy “in 
=o cury of | in Dynes 2 aS) 2 
2 °C. cm | Erg. procm ‘| 
° | 
—76.2 1.430 | 1906.0 43.6 1.082 1280.1 
—20 1.142 1522.2 34.8 1.007 1070.2 
PAS) 1.058 | 1410.1 32.2 0.978 1011.3 
i 2s) 1.018 | 1356.6 29.4 0.948 942.7 
hs eta) 0.977 1302.2 | 28.2 | 0.934 913.2 
™* 49 0.929 ~ | 1238.7 | 26.8 | 0.916 | 879.2 
70 0.818 | 1091.0 24.8 | OFSS0Uy ea 88las 
90.5 0.763 | 1017.7 23.1 0.866 786.8 
*125 0.714 951.5 2022 0.833 706.0 
*143 0.669 | 891.5 | 18.9 | 0.816 669.7 
*152.9| 0.641 854.8 | 18.1 0.806 6465 
lala 0.576 7167.5 16.2 | 0.785 589.1 
*200.5 0.507 676.4 14.2 0.764 525.8 


Molecular weight: 172.13. Radius of the Capillary tube: 0.04638 cm.; | 
in the observations indicated by *, R | 
was 0.04352 cm.; in those indicated by 
** it was 0.04408 cm. Depth: 0.1 mm. 


Under ordinary pressure the boiling point is 223.96 C. constantly ; 

notwithstanding the great viscosity of the liquid at —76° C., it was 

yet possible here to determine the value of z evidently very exactly, 

if the time of grow ofthe bubbles was sufficiently long (ca. 40 seconds). | 
a Ee ee eee 


———— 


XV 
Methyl-Cyanoacetate: CN.CH2.CO.O(CH,). 


a | 
3 : Maximum Pressure H Surface- : Molecular 
sot eee at. | tension x Specific Surface- 
Fe fe PRRs in Erg. gravity d,.| energy # in 
& | mercury of | in Dynes pro cm’. Erg pro cm» 
e 0° C. 
6°| (2.424) | (3231.6) C41) ae 222 (1387.8) 
16 pen tats 1923.2 43.9 1.140 861.2 
1 1.362 1815.4 41.4 1.122 820.8 
i= 25-5) 1.337 1783.0 38°6 1.096 me aitile! 
50 | 1.184 1578).3' 14) 35.9 1.070 | 134.6 
70.5) 1.116 1487.7 | 33.8 1.039 | 705.4 
90 | 1.043 1390.8 | Set 1.028 666.2 
* 124.5) 0.987 1315.8 28.0 0.994 601.8 
* 153.1) 0.877 1169.2 24.8 0.965 543.7 
* 176.5] 0.789 ae LOS 2ha Sy 22.3 0.942 496.8 
Selo 0.713 Oo IRS Ira 20.1 0.921 454.6 


Molecular weight: 99.05. Radius of the Capillary tube: 0.04638 cm.; in 
the observations indicated by *, R was: 
0.04352 cm., in those with “, it was: 
0.04408 cm. 
Depth: 0.1 mm. 


The carefully dried ether boils constantly at 203° C.; at — 76? C.the 
liquid is extremely viscous and gelatineous; although the time of 
formation of the gasbubbles was about 100 seconds, the viscosity in 
this case evidently diminishes the exactitude of the determinations of . 
The specific gravity 40 was at 25° C.: 1.0962; at 50° C.: 1.0698; at 


75° C.: 1.0438; at £°: 40 = 1,1231—0,001086 ¢ +- 0,0000004 ¢?, 


XVI. 

Ethyl-Cyanoacetate: CN. CH,.CO.O(CjHs). 

ovo . 
| 5 . | Maximum Pressure H Surface- ate Molecular 

se = tension x Pecite Surface- 
a inmm.mer- | | in Erg. pro | gravity d,, | energy » in 

= cury of in Dynes cm? | Erg. pro cm?, 
ol 0? ‘G 
|-17° 1.313 1750.8 39.9 1.099 876.1 

i) 1.245 1660.2 37.8 1.082 838.6 

ieee) W222: 1628.8 35.2 1.056 7193.7 
pareetaygs) 1.188 1583.5 34.2 1.046 776.1 

49 1.083 1444.5 32.8 1.032 ible SD 

71 1.016 1354.0 30.7 1.009 713.6 
| 90 0.951 1267.8 28.7 0.990 675.6 
mle 0.896 1194.8 25.4 0.955 612.4 
P13 0.803 1070.8 ~ Bes 0.927 558.3 
*176 0.727 969.7 20.5 0.904 512.7 
* 201 | 0.651 868.6 18.3 0.879 466.3 


Molecular weight: 113.07. Radius of the Capillary tube: 0.04638 cm.; 
in the observations indicated by *, R 
was 0.04352 cm.; in those by **, it was: 
0.04408 cm. 

Depth: 0.1 mm. 


The compound boils at 206° C. constantly; at —76° C. it becomes 
glassy and crystallizes very slowly on heating. The crystals melt at 
about — 40° C. The specific gravity at 25° C. was: 1.0562; at 50°C: 
1.0307; at 75° C.: 1.0052; at ¢-: A40 = 1.0817—0.00102 ¢, in general. 


O79 


XVII. 
Propyl-Cyanoacetate: CN.CH,.CO.O(C3H)). 
E ; Maximum Pressure H | Surface- | j Molecular | 
So ae ee tension 7 Specific Surface- | 
Be inmm., mer aa in Erg. pro | gravity do | energy / in 
3 cury of | in Dynes a) Erg. 2, 
2 0c. cm rg. pro cm 
—16° 1.236 1647.3 37.5 | 1058; > 91259 
0 1.184 | 1578.3 35.9 | 1.042 882.9 
P25 1.164 1551.7 3350) 1.021 835.1 
heels) 1.130 1506.5 | 32.5 1.011 815.5 
hee 1.075 1433.8 | 31.0 0.996 786.0 
ab! 0.961 1280.71, =} 29.1 0.976 747.6 
| 114.5} 0.834 W225) 92522 0.933 667.1 
2.5 0.858 | 1144.4 | 24.3 0.923 647.9 
*152.5 0.780 1039.9 22.0 0.896 598.3 
“176.1 0.701 934.6 | 19.7 0.872 546.0 
*201 0.624 | 831.8 17.5 0.847 | 494.1 
Molecular weight: 127.08. Radius of the Capillary tube: 0.04638 cm.; 
in the observations, indicated by *, the 
radius was: 0.04352 cm.; in those with 
“it was: 0.04408 cm. Depth: 0.1 mm. 
The substance boils at 216° C. constantly; at —79° it solidifies 
slowly to a crystal-aggregate, which melts at about — 39° C. The 
density d,. was at 25°C.: 1.0214; at 50° C.: 0.9973; at 75° C.: 0.9717. 


| at AG: 40 = 1,0424 —0.000962 ¢-+- 0,0000012 &. 


XVIII. 
Butyl-Cyanoacetate: CV.CH2.CO.O(C4Hb). 


vo . 
ae Maximum Pressure Surface- ey Molecular 
BY = — tension % Lo iay Surface- 
a _ jin mm. mer- in Erg. pro | gravity d energy v in 
E-= | cury of in Dynes 2 3 ce 2 
2 0°'C. cm’. Erg. pro cm». 
° 
—21.3 1.213 1617.5 35.2 1.041 928.8 
0 1.159 1545.2 33.6 1.020 898.7 
psa 1.117 1489.0 31.7 0.998 | 860.3 
if 45.2 1.055 1406.2 29.9 0.978 822.5 
im 14.9 0.975 1300.6 Alot 0.952 715.8 
* 94. 0.924 1231.6 26.2 0.934 743.2 
114.5 0.852 1135.3 24.6 0.915 707.4 
135 0.797 1063.3 23.0 0.895 671.2 
161.1 0.729 971.9 21.0 0.870 626.3 
192.1 0.662 883.1 | 19.0 0.840 | 578.4 
213.1 0.615 820.0 17.6 } -0.820! || ° 544.5 


Molecular weight: 141.1. Radius of the Capillary tube : 0.04439 cm.; i 
in the observations indicated by * it was: 
0.04352 cm. Depth: 0.1 mm. 
The ether boils at 230°.5 C. constantly; it can be cooled as far as 
—80° C., without crystallisation setting in. The specific gravity 40 


is at 25° C.: 0,9978; at 50° C.: 0.9749; at 75° C.: 0.9518; at f° it is: 
d 40 = 1.0204—0.000904 ¢ +- 0.00000016 &. 


XIX. 
lsobutyl-Cyanoacetate : CN.CHp. CO. O(CHp. CH. (CHs3)s). 


uv . 
E : Maximum Pressure 7 Surface- 3 Molecular 
eS | Ae = tension Suen: Surface- 
o. jin mm. mer- in Erg. pro ravity d energy » in 
E= cury of in Dynes cm? 3 AS. Ete epro Gale 
= 0° C. ae ; 
° 
—20.5 1.179 1572.4 34.2 1.033 907.1 
0.3 1.122 1495.9 32.5 1.014 872.7 
e225) 1.069 1424.6 30.3 0.990 826.7 
pedo 1.013 1351.1 28a 0.971 793.3 
* 74.8 0.934 1245.4 26.4 0.944 743.6 
* 04.5 0.879 1174.6 24.9 0.925 710.9 
| 115 0.811 1081.3 23.4 0.905 677.9 
| 135.1 0.757 1009.2 21.8 0.886 640.5 
161 0.686 914.6 19.7 0.862 589.5 
191.8) 0.595 792.9 17.0 0.834 520.0 
213 0.541 720.9 15.4 0.815 478.4 


Molecular weight: 141.1. Radius of the Capillary tube: 0.04439 cm.; 
in the observations indicated by *, Rwas: 
0.04352 cm, 
Depth: 0.1 mm. 

The compound boils at 223° C. constantly; it can be undercooled 
as far as —76° C,, and crystallizes then slowly into a crystalline 
aggregate, melting at about -—26? C. The specific gravity at 25’ C. 
was d,,. = 0.9903; at 50° C.: 0.9669; at 75° C.: 0.9441. At ¢° it is 


generally : Ayo = 1,0138—0,.000952 ¢ + 0.00000032 @. 


XX. 
Amyl-Cyanoacetate: CN .CH,.CO.O(C;H\). 
5 Maximum Pressure Surface- Pes Molecular 
pho FS RE ae eee ad eet aa Specific Surface- 
Go i energy 
= en in Erg ravity d : 
E-= | mercury of | in Dynes pro cm?, ier IS Sy 18 
a 0° C. pro cm’. 
a SSS SSS = — WSS SS ——————————————_SI ESSE 
—17:5| 1.080 1440.3 32.7 1.017 933.5 
IS 1.029 1371.3 SI 1.001 897.2 
ee Zee 1.028 1370.2 29.5 0.976 865.5 
aD) 1.000 1333.2 28.7 0.966 847.9 
69 | 0.880 1172.9 26.5 0.939 797.8 
89 | 0.831 1108.3 25.0 0.920 763.0 
plas) 0.807 1075.4 Poel 0.891 107.7 
153 0.744 992.6 21.0 0.864 668.3 
0.689 919.1 19.4 0.843 627.6 
201 0.634 845.6 17.8 0.821 586.1 
| 


Molecular weight: 155.11. Radius of the Capillary tube: 0.04638 cm.; 
in the observations indicated by *, R was 
0.04352 cm.; in those with * it was: 
0.04408 cm. 
Depth: 0.1 mm. 


The compound boils at 240°.2C.; at —76°C. it is a jelly, but does 
not crystallize. The specific gravity at 25° C. was: 40 = 0.9763 5 
|) Yat 50>'G:: (0/9547; at 715° G2 O82, Ate itis: A4o = 1.0019—0.090061 z 
+ 0.00000032 #. 


Molecular Surface 
Energy in Erg. pro cm’. Fig. 5. 


4SO 
-50°60"-40"-20° 0° 20° 4W° 60° 80° 100" 120° 14° 160° 180" 200.220 }eMperature 


XXI. 
| Trichloromethane: CHCl. 


Maximum Pressure Surface- 
tension x 


| Molecular 
| Specific | Surface- 
| in mm. | in Erg. Se ee uP RCHCRY 
| mercury of | in Dynes | pro cm? | gravity “4°! in Erg. 
! = 


| Temperature 
iba © (CG, 


OnE: | | pro em?2. 


—22 1.142 | 1523.4 | 32.5 1.555 | 587.5 
0 | 1.050 1394.3 29.7 1.519 545.3 
25 | 0.927 1236.0 | 26.2 1.476 490.4 
35 | 0.881 |) Lae S 24.8 1.459 467.8 
55 | 0.798 1063.9 22.4 1.425 429 .2 


Molecular weight: 119.51. Radius of the Capillary tube: 0.04385 cm. 

| Depth; 0.1 mm. 
The trichloromethane was prepared from purest chloral, carefully 
| dried, at —79° C. several times frozen, and purified by repeated 


distillation. It boils constantly at 61°.2 C.; at this temperature, the 
value of x is: 21,8 Erg. pro cm?. 


382 


XXII. 
Tetrachloromethane: CCl. | 
| 
£ | Maximum Pressure H | Surface- aa Molecular 
go a = _____} tension x Becmc Surface- 
a. in mm. mer- E in Erg. pro | gravity d,.| energy “in 
| = | cury of | in Dynes cm?, 4° Erg. pro cm’, 
= | OG. 
—18° | 1.087 | 1450.4 | 30.9 1.659 633.0 
0.1) 1.005 1340.9 28.5 1.632 590.2 
25 | 0.899 1199.5 25.4 1.585 536.4 
35 | 0.862 1149.4 | 24.3 1.560 518.6 
55 0.793 1058.1 22.3 1.525 483.2 
| 1 ie - ee. ase 
Molecular weight: 153.80. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 
Under reduced pressure (ca. 90 mm.) it boils at 26° C., and solidifies 
at — 60’ C. to a white crystalline mass. Under ordinary pressure, it 
boils constantly at 76°.4 C. At this temperature the value of x is 
about: 20.2 Erg. pro cm?*. 
—4 
Molecular Surface-Energy 
in Erg pro em’. Fig. 6. 
7020 
990 
960 
aS 
930 TAN 
PAO 
900 NESS 
8 YO 
a70 SEO RR 
oh Na NG 
; ‘Sa, NRG? 
750 ~S ‘WS 
720 SSE RY 
a RES SENG 
690 SS Oe Nah 
660 GENS. SS 
630 SNORE OS 
\ SSS aN 
600 FSS NS Ye 
570 Ns We Se 
500 Se x 
> ? uN \’ 
510| tx CancacHiale® WO, 
480 AS 
450 : aot 
SO OPI WO 20° YO” OF 80 100 120 M0 160 180 200 220° 200 260" “NPE 


rature 


383 


XXIIL 


Isobutylbromide: (CH3). CH . CH2B?). 


= 4 Maximum Pressure H Surface- Specif Molecular 
so : tension x | ~Pectlic Surface- 
os in mm, mer-| . inErg. pro | gravity dg. energy “in 
“ cury of in Dynes cm?. Eeonocotenall 
= One: ot 
= ] — =z = <== SS SSS SE —— = = = = = — 
L95” 1.227 1636.5 38.4 1bS85 ma eeS2166 
—19.5 0.949 1265.9 29.5 1.314 653.7 
0 0.874 1166.0. | 27.1 1.291 607.6 
25.4 0.790 1053.5 24.4 1.259 556.3 
44.4, 0.728 970.2 22.4 | 1.236 By eie} 
69.9, 0.646 861.9 19.8 1.205 464.8 
85.3 0.600 799.5 18.3 | 1.186 439.2 


Molecular weight: 137.07. 


Radius of the Capillary tube : 0.04803 cm. 


Depth: 0.1 mm. 


The carefully dried compound boils very constantly at 90.°5 C.; at 
this temperature x is about 17.9 Erg. pro cm?. 


Molecular Surface- 


Energy in Erg pro cM?. 


Vig. 7, 


-§0°-60°-40° 20° O° 20° 40° 60° 80°10" 


Temperature 


| 
| 
| 


§ 5. 


384 


Temperature-coefjicients of w of the here studied substances. 


norm. Propylalcohol. Isobutylalcohol. 
Temperature-interval: re in Erg. Temperature-interval: = in Erg. 
between —76° and —21° 1,78 between —71° and — 12° 2,3 
—21° , +259 1,11 —12° ,, +101° 1,1 
2 ap 91° 1,10 
Diethylether. Ethylf ormiate. 
between —75° and —20° 2,16 between —76°,5 and —16° 1,72 
—— 2) ae 0? 1,94 —16° ,, +25° 1,62 
O20 ay. 29° 1,70 Zoe ss 35° 1,29 
Se 54° 1,12 
Ethylchloroformiate. Ethylacetate. 
between —75° and —21° 2,86 | between —74° and 0° 2,50 
—21° , +25° 2,41 Og. 25° 2,37 
Dock TOS 1,82 Dap 35° 1,86 
WY 91° 1,70 GI? 5) 55° 1,78 
55°u,. nis 1,30 
Methyl-Isobutyrate. Ethyl-Isobutyrate. 
between —73° and —219,5 3,0 between —78° and +109? 2,15 
—21° , 25° 2,4 ; 
Pao 45° 2,1 
452), 91° 1,7 
Isobutyl-Isobutyrate. Acetone. 
between —76° and — 21° 3:2 between —73° and —19°,5 1,81 
—21° ,, +135° 2,18 —19° 5, =e 1,66 
Oy 54° 1,57 
Methylpropylcetone. Ethyl-Acetyloacetate. 
between —74° and 0° 2,13 between —20° and +-176° 2,19 
2 5) g9° 1,73 
Methyl-Methylacetyloacetate. Ethyl-Propylacetyloacetate. 
between —71° and —21° 3,39 between —76° and —20° 3,74 
Al 0° 2,47 —20°,, +20° 2,84 
WH 70° 2,18 beer. 70° 2,36 
TOR! Sf 156° 1,94 TPs ies 2,24 
12525 eee OSS 2,11 
Then an increase: 2,37 to 2,68, occurs 
as a consequence of beginning dissociation. 
Methyl-Cyanoacetate. Ethyl-Cyanoacetate. 
between —76° and — 16? not measurable | between —-17° and +201° 1,88 


independently of 


viscosity. 


—16° ,. +1979 


1,90 


Propyl-Cyanoacetate. | Butyl-Cyanoacetate. 


ete Ou. . Ou. 
Temperature-interval: ay in Erg. Temperature-interval: a in Erg. 


between —16° and +152? 1,88 ‘between —21° and 4213° 1,62 
Then an increase: 2.13, under dissoci- 
ation and liberation of HCN. 


Isobutyl-Cyanoacetate. | Amyl-Cyanoacetate. 
between —20° and 0° 1,64 | between —17° and 4- 1° 2,0 
Ps 1152 1,70 | 1 201° ca: 1,6 


i taee 213° 2,0 
Gradual decomposition, under liberation | 


of HCN. | 
Chloroform. Carbontetrachloride. 
between —22° and --55° 2,06 between —18° and 0° 2,6 
Ore; 25° 1,95 
25° 55° 1,75 
Isobutylbromide. 
between —75° and —19° 3,0 


alig2 9, -1-952 2,15 
25°, = 699,9_—s—«2,08 
70°, 90° 1,91 


acy 0 
Evidently only in some cases the coefficient 5, appears to be really 


constant; in most cases it decreases doubtless with a rise of tempe- 


rature. Where the inverse behaviour was stated, a decomposition of 


Oo 
the studied substance always seemed to occur. The value for - 
t 


is in the interval of ordinary temperatures relatively small for propyl- 
and isobutyl-alcohol and for the cetones; however in these cases it 
appears to be variable with the temperature in no higher degree 


0 
than in the cases, where the values of = do not differ largely from 


2.0 Erg. 
Groningen, June 1914. Laboratory for Inorganic Chemistry 
of the University. 


386 


Chemistry. — “The Temperature-coefficients of the free Surface- 
energy of Liquids, at Temperatures from —80° to 1650° C. 
III. Measurements of some Aromatic Derivatives.” By Prof. 
Dr. F. M. Jarcer and M. J. Surv. (Communicated by Prof. 
P. vy. Rompuran). 


§ 1. In continuation of our measurements of organic liquids, the 
data obtained in the study of a series of aromatic compounds, are 
reviewed here in tables, quite in the same way as in our former 
communications’). This series of substances includes the following terms: 

Nitrobenzene; ortho-Nitrotoluene ; Aniline; Dimethylaniline ; ortho- 
Toluidine; Thymol; Methyl-, Ethyl-, and Benzyl-Benzoates ; Salicylic 
Aldehyde ; Acetophenone, and the non-aromatic compound: e-Cam- 
pholenic Acid. 

With respect to the determination of the specific gravities and the 
purification of the studied substances, we can refer to the preceding 
communication; the diagrams also have the same significance, as 
indicated there. 

§ 2. Aromatic Derivatives. 

1. 


Nitrobenzene: C,H;(NO,). 


5 Maximum Pressure 1 | Surface- | Rae Molecular 
| id | tension x | ~Pecic Surface- 
| Sey he in Erg. pro | ity d energy “in 
= in mm. mer-| ; | Sravity 
=~ cury of 0?C.| '" Dynes cm? 4 Erg. pro cim?. 
5 1.538 | 2050.5 | 44.4 1.215 064.7 
26.6 1.473 | 1965.8 | 42.5 1.197 932.7 
| 34.9 1.448 | 1930.5 41.7 1.190 918.7 
55.3 Lon 1827.8 | 39.5 1.171 879.7 
70.8 1.314 1751.8 37.8 1.156 849.0 
100 1.198 1596.0 34.4 1.125 786.8 
110 1.156 1541.6 33.2 1.115 _ 163.9 
126 1.089 1459.8 31.4 1.097 730.4 
145.5 1.014 1351.9 29.0 1.075 683.7 
W225 0.903 1204.0 25.8 1.042 621.0 


Molecular weight: 123.06. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 


The nitrobenzene was carefully dried, several times frozen, and 
distilled; it boils at 209° C. constantly. At this temperature 7 = 21.2 
Erg. pro cm? At O° C. it solidifies completely. The specific gravity 
at 25° C. is: d4. = 1.1988. 


1) F. M. Jaraer and M. J. Sarr, Preceding communication, (1914), 


Il. 


Ortho-Nitrotoluene: CH; .C ,H,. (N02). 
(1) (2) 


© } Maximum Pressure // Surface 
30 = _ tension x 
a | in mm. mer- in Erg. pro 
Es cury of in Dynes eat 
O2NG; 
0.1 1.505 2006.8 43.3 
9.6 1.465 1953.1 42.1 
zo 1.416 1887.5 40.9 
3438 1315 1833.1 39.7 
* 49.3 1.257 1675.8 38.2 
70 1.252 1669.4 35.8 
101.6 1.132 1509.8 32.4 
122.6 1.055 1406.5 30.1 
144 0.971 1295.4 Qe 
148.6 0.954 1272.4 27.2 
170 0.864 1151.9 24.5 


Molecular weight: 137.1. 


The compound boils at 218° C. constantly; the meltingpoint is 
— 4° C. At the boilingpoint, the value of x is about 18.1Erg. pro cm’. 


0.04408 cm.; 


0.04638 cm. 
Depth: 0.1 mm. 


Specific 
gravity a4, 


ee ee 
_ 
—_ 


Radius of the Capillary tube: 0.04385 cm.; 
in the observations, indicated by *, R was 
in these with 


Molecular 
Surface- 
energy » in 
Erg. pro cm>,| 


DOW bNWOWWH oo | 


it was: 


Il. 


Aniline : CgH;(N H2). 


E : Maximum Pressure H Surface- 
a ———| tension , 
Yo : lire! 

a in mm. | in Erg. pro 
££ | mercury of in Dynes antl 
fe O3E 

(e) 

0 1.573 2096.5 45.4 

5.3 1.552 2069.8 44.8 
26.2 1.473 1963.8 42.5 
34.7 1.452 1935.8 41.8 
54.8 1.371 1827.8 39.5 
70 1.320 1759.8 38.0 
100 1.190 1586.5 34.2 
109.5 1.156 1541.6 382 
126 1.089 1459.8 31.4 
143 1.027 1369.2 29.4 
148.8 0.998 1331.8 28.6 
173.7 0.889 1185.8 25.4 


Molecular weight: 93.04. 


_The liquid boils at 184° C. constantly. It is colourless, and only at 
higher temperatures it gets somewhat yellowish. At the boilingpoint, 


x is: 24.3 Erg. pro cm? 


Radius of the Capillary tube: 0.04385 cm. 


Depth: 0.1 mm 


| 


Specific 
gravity a4, 


Molecular 
Surface- 
energy / in 
Erg. pro cm’. 


IV. 


Dimethylaniline 5 CoHs 5 N(CH3)3. 
| wo 7 
(ees Maximum Pressure Surface- ; Molecular 
HS) st sf | @tensionie Specific Surface- 
oo : | = z 4 energy » 
= eee in Erg. ravity d. : 
== | mercury of | in Dynes pro cm?, SEE By Erg. 
i= OPC, pro cm?. 
26 | 1.165 1553.2 36.6 | 0.951 926.4 
45.5 | 1.087 1449.1 34.1 0.935 873.0 
| 66.5 1.018 S579) 31.9 0.917 827.3 
| 86.5 | 0.959 | 1278.4 30.0 0.900 787.8 
| 106 0.893 1190.8 271.9 0.884 741.5 
125.8 0.831 1107.6 25.9 0.867 697.3 
146 0.768 1024.4 23.9 0.850 652.0 
166 9-709 945.3 22.0 0.832 608.8 
184 0.650 866.1 20.1 0.817 | 563.0 
Molecular weight: 421.11. i) Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 
The liquid boils at 191° C. constantly; it solidifies easily and the 
crystals melt then at 0°.5 C. The value of x at the boilingpoint is 
about: 19.3 Erg. per cm?.. 


Molecular Surface-energy 
in Erg pro em’. Fig. 1. 
7170 


450 
“S§0°-60°- 40° 20° O° 20° 40° 60° 80° 100°/20° 740° 160° 150° 200° 220° 


389 


V. 
Ortho-Toluidine: CH, .CgH,.(NH,) . 
(1) (2) | 
E ; Maximum Pressure 1 Surface- : Molecular 
aU z= se tension x Specific Surface- 
oe . . . 
&_ jin mm. mer- in Erg. pro | gravity d energy in 
Es cury of in Dynes ane. Se aa4e Erg. pro cm? 
5 a: ‘ 
= ORNS | 
—20° 1.573 2098 .0 | 45.4 1.027 1005.8 
0.6 1.492 1989.1 43.0 1.013 961.4 
9.3 1.465 1953.1 42.2 1.006 947.9 
25 1.403 1870.5 40.4 0.992 | )ikeyGE) 5 
34.6 1.375 1833.1 39.6 0.985 902.1 | 
50.1 1.310 | 1765.8 Sileu 0.973 | 865.8 | 
70.5 1.234 | 1645.2 39,0 0.957 | 824.4 
101.4 ielS3 151025 S285 | 0.933 767.6 
123.2 1.043 1391.0 29.9 0.916 714.9 
144 0.957 1277.0 27.4 | 0.899 663.3 
149.5) 0.937 1249.8 26.8 0.895 650.8 
172 0.831 | 1108.2 Zoe 0.877 583.3 


Molecular weight: 107.09. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 
The ortho-toluidine boils at 197.4 C. constantly. It is perfectly 
colourless, but above 180° C. it gets gradually reddish brown. At 
the boilingpoint 7 = 19.9 Erg pro cm’. 


VI. 


Thymol : (CH;),CH. CsH;. OH(CH3). 


& Maximum Pressure H Surface- | eer Molecular | 
EO) 5 || ea ok ees tension z% Wael te Surface- | 
Vo 5 : : 
a jin mm. mer- in Erg. pro itv d energy / in 
5 . gravity | 
E ¢ vary ot IPRS cm?, bk Erg. pro cm*: 
g° 1.176 | 1567.9 34.2 0.986 975.1 
25 1.109 1478.5 32.2 0.968 929.4 
45.7 1.054 1405.7 30.6 0,952 893.1 
710.7 0.991 1321.9 28.6 0.933 846.0 | 
90.1 0.943 1257.0 27.3 0.920 815.2 | 
115 0.875 1156.6 ZOE 0.901. 766.0 
135.3 0.825 1099.3 23.8 0.887 728.2 
“160 0.703 935.9 21.9 0.867 680.3 
)* 190.1 0.628 837.0 19.5 | 0.845 616.2 
er 0.578 770.3 17.9 0.829 572.9 
Molecular weight: 150.11. Radius of the Capillary tube: 004439 cm. ; 
in the determinations indicated by *, R 
was: 0.04803 cm. 


Depth: 0.1 mm. 


The substance melts at 51°.5 C., and boils at 231.°5 C. constantly ; 
it can be undercooled to a high degree. At the boilingpoint ~ is 16.6 
Erg. The specific gravity at 24.°4 C. is 0.9639. 


Ww 
co 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


390 


VII. 


& Maximum Pressure 
10) 
D0 7 
| ES in mm. mer- sa AGS 
2 cury of 0° C. y 
| | 
le? 1.405 1873.1 
S25r1 1.306 1741.2 
| 245) e222 1629.2 
tas: || 1.110 1479.8 
*04.5| 1.034 1378.7 
115.2 0.946 1261.2 
135.3] 0.875 1166.9 
(160 | 0.791 1054.6 
192.5 | 0.686 914.6 
I 
| D 


Methylbenzoate: C,H,;.CO. O(CH;). 


Surface- 

tension x 
| in Erg. pro 
cm*. 


Specific 
gravity ayo 


Molecular 
Surface- 
energy “in 
|Erg. pro cm2, 


| 


—KMNMMMWWwWwFt | 
SCnanorhaA- 
ADWRhREADWS, 


epth: 0.1 mm. 


Molecular weight: 136.06. Radius of the Capillary tube: 0.04439 cm.; 
in the observations indicated by *, the 
| radius was: 0.04352 cm. 


The boilingpoint of the compound lies at 195.°2 C. The liquid can 
be undercooled as far as —21° C.; then it crystallizes, and the crystals 


/ 


melt at about —15 C. Atthe boilingpointthe value of , is: 19.4 Erg. pro cm’. 


Specific 
gravity Ayo 


Molecular 
Surface- 
energy vin 
Erg. pro cm:. 


1.081 
1.066 
1.047 
1.032 
1.009 
0.995 
0.980 
0.964 
0.945 
0.921 
0.914 


1045.7 
1001.3 
947.7 
904.3 
833.8 
782.1 
738.5 
694.6 
624.7 
554.9 
539.7 


adius of the Capillary tube: 0.04439 cm. ; 


in the observations indicated by * this 


VIL. 
| Ethylbenzoate: CyH;.CO. O(C:Hs). 
E J | Maximum Pressure H Surface- 
sos tension 7 
Heese in Erg. per 
| Se ht - : 
| =.= jin mm. mer-| . f 
&  jcury of 0° C.| in Dynes cm’. 
Pabete eat | | aw 
550-51) Absssun| wuireses 39.0 | 
0 | Lei) | 1694.1 | 37.0 | 
be ay | 1.213 1617.6 34.6 
* 45.1) 1.148 1530.4 S2ai 
he ztey | 1.044 | 1392.4 29.7 
* 04.4 0.972 | 1295.9 27.6 
114.6 0.892 1189.4 25.8 
| 135.4| 0.833 | 1110.6 24.0 
160.2) 0.740 986.7 21e3 
| 192.1] 0.649 | 865.0 18.6 
| 200 0.628 | 838.0 18.0 
—— — — = —< = | — 
Molecular weight: 150.08. R 
radius was: 0.04352 cm. 
| The compound boils at 210.°8 C. It can be undercooled as far as 


—79' C., and then slowly crystallizes to a white mass, which melts 


at —57? C. At the boilingpoint, z is 17.4 Erg. pro cm*. The great 
viscosity ofthe liquid at -70° C. makes accurate measurements impossible. 


391 


IX, 
Benzylbenzoate: CoHs CO _O(CH . CzHs). a ae 
8) . 
ae Maximum Pressure 1 Surface- feline Molecular 
Bo. a =| satensionyy peene Surface- 
Be in mm. mer- | in Erg. pro | gravity d,, | energy ” in 
= cury of in Dynes 2. Erg. pro cm’. 
EB 0°C. Wee Be 
51-8). 1.622 2162.4 | 47.4 1.153 1533.2 
0 1.548 2063.5 45.2 1.136 1476.6 
25 1.456 1941.9 42.5 oye) 1405.7 
45 1.384 1851.8 | 40.5 1.099 135235 
710.8 1.294 1725.8 37.6 1.078 1271.9 
90.8 1.230 1640.0 35.8 1.062 Wn eli22se2 
106.2 1.179 1572.4 34.3 1.042 1186.9 
135.1 1.092 1455.2 Slei 1.027 1107.6 
*159.9 0.949 1265.9 29.8 1.006 1055.6 
“190 0.890 1186.7 27.9 0.982 1004.4 
S215 0.849 1132.6 26.6 0.965 968.8 


Molecular weight: 212.10. Radius of the Capillary tube: 0.04439 cm.; 
in the observations indicated by *, this 
radius was: 0.04803 cm. 

Depth: 0.1 mm. 

The substance boils constantly at 308°? C.; it can be undercooled 
as far as — 70? C., and then crystallizes. The meltingpoint is some- 
what higher than -++ 12° C. At the boilingpoint % is 22.6 Erg pro cm’. 
The density at 25” C. is: Ayo = 1.1151; at 502 C.: 1.0940; at 75° C.: 


1.0724; at PC: Ayo= 1.1357 — 0.000814 ¢. 


ee 


X. 


Salicylic Aldehyde: C,H,.COH, 


| 
: p | Maximum Pressure H Surface- Specifi Molecular 
hag = oa tension x Decne Surface- 
| es in ae Wee ‘gras in eS pro | gravity dg. ety yn i 
2 et cm? rg. pro cm*. 
0 1.534 2045.5 44.8 1.176 989.4 
25 1.443 | 1923.8 42.1 1.152 942.6 
45.5 1.368 1823.8 39.9 1.132 903.9 
70.7) 1.274 1698.6 STL 1.108 852.5 
90.5 1.205 1606.5 35.0 1.090 813.1 
116.2) 1.115 1486.8 32.4 1.066 764.0 
135.4 1.053 1403.8 30.6 1.052 127.9 
“160 0.896 1195.1 28.1 1.030 677.9 
1909 0.796 1061.9 24.9 1.002 607.2 


-- ——+-- a ——— ——— il — ——-~ = - —-—--— —~—— = — 
Molecular weight: 122.05. Radius of the Capillary tube: 0.04439 cm. ; 
in the with * indicated observations, this 
radius was: 0.04803 cm. Depth: 0.1 mm. 
The boilingpoint is constant at 192.°5 C.; the substance soon solidifies, 
and melts at —7> C. At 25° C. the specific gravity is: dy. = 1.1525; 
at 50 C.: 1.1282; at 75° C.: 1.1036. At ¢ in general: a4, = 1.1765— 


0.000954 t—0.00000024 ¢?, At the boilingpoint, the value of x is: 25.4 
Erg. pro cm?, 


26* 


392 


XI. 
Acetophenone: CH;.CO. CgHs. 
ea ie, | 
E | Maximum Pressure 1 Surface- ent Molecular 
sO |= 2 at AA tension, Pecuic Surface- 
&° jin mm. mer. | in Erg. pro | gravity d,, | energy vin 
E-= | cury of | in Dynes cm’. ‘Erg. pro cm®. 
24.8| 1.375 1833.6 40.1 1.024 963.5 
44.7 Meo 1703.1 37.2 1.007 903.8 
71 1.169 1558.9 34.0 0.984 839.1 
90.3) 1.098 1464.2 31.9 0.967 796.3 
117 1.017 1356.2 29.5 0.945 747.8 
135.3) 0.966 1288.6 | 28.0 0.929 717.9 
*160 0.824 1099.3 | 25.8 0.907 672.1 
*189.9 0.750 999.4 | 23.4 0.881 621.5 
*200 | 0.728 970.2 | 225i 0.872 607.1 
“Molecular weight: 120.06. Radius of the Capillary tube: 0.04439 cm. 


in the observations indicated by *, the 
radius was: 0.04803 cm. 
Depth: 0.1 mm. 

The compound boils constantly at 201. 5 C.; and becomes solid at 
—20° C.; it melts at + 20°.5 C. At the boilingpoint the value of x is 
22.6 Erg. pro cm*. The specific gravity at 25° C. is: ayo = 1.0236; at 

| 502 C.: 1.0026. 


XII. 
| (CH,).:C.CH.CH, COOH. 
| @-Campholenic Acid: |. >CHe 
(CH,).C: CH 
| . Nl al | oz 1 pa a . z 
E : Maximum Pressure H | Surface- | ane Molecular 
SS peste ie —| tension x peeilic Surface- 
a. — |in mm. mer- in Erg. pro | gravity d, | energy # in 
Wes eee Pe ate Os in Dynes cm’. Erg. pro cm’, 
ie = ole eOSIC a | Lane 
—19.8 (1.695) (2259.8) (52.6) | 1.030 (1598 .6) 
1.177 1569.2 | 37.0 1.016 1114.1 
25 1.077 1436.6 33.8 | 0.999 1029.4 
45.4 1.019 1358.5 319 0.985 980.9 
TOA Wscke |) 12D 29.8 | 0.969 926.6 
85.3 0.915 1220.1 28.6 0.960 895.0 
P| 0.846 | 1128.5 26 4 0.939 838.7 
138.1} 0.805 1073-2 25.1 | 0.925 805.6 
156 | 0.771 1027.9 | 24.0 | 0.913 771.5 
2A 0:728 | 970.2 22.6 0.902 739.1 
191.7 0.664 885.2 20.6 0.889 680.5 
212 | 0.608 810.6 | 18.8 0.876 627.8 
————— - ae . a No ee ee eee ee 
Molecular weight: 168.13. Radius of the Capillary tube: 0.04803 cm. 
Depth: 01 mm. 


Under a pressure of 12 mm., the compound boils constantly at 
153° C. Below 0° C. the liquid is extremely viscous; although the 
growing of the gas-bubbles lasted about 50 seconds, the measurements 
at —19°C. cannot be considered to be very reliable. The substance 
| solidifies at —79 C.; above 160°C. it gets yellow by aslowly proceed- 
| ing decomposition. 


— — 


Molecular Surface-energy 
in Erg pro cm? 
Fig. 2. 


I00 
40°-20° O° 20° 40° 60° SO° 700° 720°740°760° 180° 209° 220° 


§ 3. Values of the Temperature-coefficients of the molecular 
Surface-energy |. 


394 


Nitrobensene. 


0 | 
Temperature-interval: a in Erg: 
t 


between 5° and 35° 1,53 
SOC aml 1,93 
TAI able 2.16 
WDD ee 2,25 
145099, else 2,31 
Aniline. 
between 0°? and 35° 1,57 
Sole OS 1,73 
102 AS 2,16 
o-Toluidine. 
between —20° and +-101° 1,98 
LOC 144° 2,44 
14420 WP? 2.85 


Above 1602 a graduél decomposition 
with colouring of the liquid, sets in. 


Methylbensoate. 

between 0° and 25° 3,0 

DOR MEADS 2,6 

45° >= 192° 2,21 
Bensylbenzoate. 

between —22° and -+-135° 2,70 

135omer 160° 2,08 

160°, 211¢ 1,66 
Acetophenone. 

between 25° and 45° 2,99 

RSD ee Ale 2,45 

TEE, OS 2,19 

90°, 160° 1,76 

16025 7,7 #2002 1,61 


o-Nitrotoluene. 


Ou 
Temperature-interval: va in Erg: 
t 
between 0°? and 25° 1,81 
BRP 7 282 2,19 
492 232 2,29 
1232 8 4a 2,42 
144° , 170° 2,82 
Dimethylaniline. 
between 26° and 46° 2,12 
AGS fyi 2,23 
Thymol. 
between 0°? and 160° 1,83 
16025 sez 2,09 
Ethylbenszoate. 
between —20° and +200° 2,29 


Salicylic Aldehyde. 


0° and 160° 
160° , 190° 


between 1,98 


2,19 


a-Campholenic Acid. 
between —19°,8 cannot be determined 


and 0° independently of 
the viscosity 
GF Aye 3,39 
25°, «45° 2,42 
45°, 85° 2,12 
852 ele 1,76 
117° ,:138° 1,59 


Above 138° (decomposition) ca. 2,6 


3esides some straight lines, there are found here several curves 


for 


the dependence of « and ¢, showing in contradistinction with 


the formerly deseribed ones, the shape of that of wuater. 


Groningen, June 1914. 


Laboratory for Inorganic Chemistry 


of the University. 


- 395 


Chemistry. — “The Temperature-coefficients of the free Surface- 
energy of Liquids, at Temperatures from —80° to 1650° C.: 
IV. Measurements of some Aliphatic and Aromatic Ethe:s.” 
By Prof. F. M. Jagger and Jun. Kany. (Communicated by 


Prof. P. van Rompurau.) 


§ 1. In this communication the results obtained in the measure- 
ments of the free surface-energy of a number of ethers, are recorded 
by us. With respect to the purification-methods and the determina- 
tion of the specific weights, we can refer to communication II of 
this series); also the arrangement of the data and the significance 
of the diagrams are completely the same as indicated before. 
This series includes the following aliphatic terms: 

Amylacetate ; Diethyl-Ovalate ; Diethylmalonate ; Diethylbromo- 
malonate; Diethyl-Ethylbenzylmalonate; Dimethyl and Diaethyltartrates; 
and the following aromatic substances : 

ortho-Nitroanisol; Methyl-, Ethyl-, and Phenyl-Salicylates ; Methyl- 
Cinnamylate. 


| | | 


I. 
Amylacetate: CH3.CO.0O(C;H,;). 
Semi, oe | Bir 
ee Maximum Pressure H | Surface. | : Molecular 
oe = tension x Specific | Surface- 
reecennl in Erg. pro i | energy “in 
in mm. mer-| .; : gravity d,. gy ! 
es cury of 0° C.| Ul TONES cm?. | : |Erg. pro cm?. 
| 
| | | : | a \ tie | 
| | | ; a ; 
SiN 1.099 1465.8 34.6 0.968 907.8 
ir 4 0.915 1220.1 28.7 0.918 780.0 
0 | 0.850 | 1132.6 26.6 0.896 734.9 
25.8) 0.771 | 1028.6 24.1 | 0.869 679.5 | 
46 | 0.712 | 949.4 22.2 | 0.847 636.8 
66.5. 0.653 870.3 20.3 0.827 591.6 | 
86.5) 0.600 | 799.5 18.6 0.808 550.5 
106 0.549 7132.9 17.0 0.790 510.8 
| 125 0.506 | 674.6 15.6 0.774 475.1 
| 614.6 | 14.2 0.752 | 440.9 
| 


| Molecular weight: 130.11. | Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 


The boilingpoint of the carefully dried compound lies at 148.94 C.; 
| at this temperature x is 14.0 Erg. pro cm?®. 


1) F. M. JAnGER and M. J. Suir, These Proc. (1914) p. 365. 


396 


II. 


Diethyl-Oxalate: (C2H;) 0.CO.CO. O(C)Hs5). 


| = | Maximum Pressure 1 Surface- , Molecular 

eee Reet a _ tension Specific Surface- 
a° jin mm, mer- | in Erg. pro | gravity d,. | energy » in 
E=  cury of in Dynes | em?, Erg. pro cm?.. 
oat OAC | 

—20.7| Nt rizt | 1569.9 37.0 1.139 941.0 

Om ha OU 1482.5 34.9 1.110 903.0 

26 | 1.025 | 1366.5 32.1 1.074 848.8 

| 46 om52 | «(1278.4 «| = 30.0 1.050 805.5 

| 66.7, 0.896 1195.1 | 28.0 1.025 764.0 
86.5 0.818 1091.0 25.5 1.001 706.8 
106 | 0.768 1024.4 23.9 0.977 673.3 
125) 9 0.717 955.9 22.2 0.954 635.4 
145.5 0.650 866.6 | 20.1 0.930 581.1 
166 0.568 15des 17.6 0.905 521.8 
184 | 0.478 637.3 14.6 0.883 440.0 


Molecular weight: 146.08. Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 

The substance boils at 99.°5 C. constantly, under a pressure of 

about 12 mm. In solid carbondioxide and alcohol it soon solidifies, 


and melts at —41.°5 C. Above 160? C. the ether seems to decompose 
slowly. 


Ill. 


| Diethylmalonate: (C2H5) 0. CO.CH,.CO.O(C,Hs). 


= _ | Maximum Pressure H Sur face- : Molecular 
eS eee | at ensioney Specific Surface- 
oD ie) . . . 
a” |in mm. mer- _ in Erg. pro | gravity d energy » in 
|} ££ |  cury of in Dynes em? AS Ere nco 
| 2 ole | ; g. pro cm’, 
= 
\—19.9) 1.237 1649.2 35.5 1.095 985.3 
0.7 1.167 1555.8 | Oo, 1.075 941.2 
8.5) 1.142 1523.2 32.9 1.068 928.4 
| ayy 1.077 1435.9 31.0 1.050 884.8 
| 34.5 1.044 1391.9 30.0 1.041 861.2 
50.1) 0.994 132582) 28.5 1.025 826.6 
| 69.2) 0.920 1226.8 26.3 1.005 7712.9 
10204 0.804 1071.8 23.0 0.969 692.5 
124.5 0.723 963.9 20.6 0.945 630.7 
144 0.660 880.2 18.8 0.924 584.3 
| 148.7) 0.649 866.4 18.5 0.919 571.1 
tpl | 0.571 761.6 16.2 0.896 513.9 


Molecular weight: 160.1. 


Depth: 0.1 mm. 


| 


Radius of the Capillary tube: 0.04385 cm. 


| The compound boils constantly at 197.°3 C.; after crystallisation, 
it melts at — 50° C. At 25° C. the specific gravity was 1.0518; at 50° C.: 
1.0254. At the boilingpoint the value of x is: 13.7 Erg pro cm*. 


397 


IV. 


| Diethyl-Bromomalonate: (C2H;)O.CO.CHBr. CO. O(C2Hs). 


| | 


vu . | 
= _ | Maximum Pressure /7 | Surface- | ; Molecular | 
WO = —| tension x | SSE Surface- | 
oe inmm,mer- | _ in Erg. pro | gravity d4o energy / in 
ae cury of in Dynes | cm2, | \Erg. pro cm2,| 
fe (HKG; | 
—20.7 1.250 1666.5 | 39.1 1.464 1168.2 | 
0 1.165 1553.2 36.4 1.436 | 1101.6 
26 1.065 | 1419.9 33.2 | 1.401 1021.5 
45.5 0.999 133259 Sel | © tess 968.9 
66.6) 0.943 Zoe || 29.3 1.347 | 925.4 | 
86.5 0.896 1195.1 27.8 1.320 890.0 
106.5 0.853 1136.8 26.4 1.293 } 856.9 
126 0.815 | 1086.8 25.3 1.266 | 832.8 
| 146 OF780) Fa 103959 24.2 1240 807.7 
i 


Molecular weight: 239.09. Radius of the Capillary tube: 04803 cm.; 
Depth: 0.1 mm. 


Under reduced pressure (ca. 20 mm.) the substance boils constantly 
at 121° C.; at —54> C. it becomes a jeily, but does not crystallize. 
Above 150° C. it begins to be tinged brownish, apparently by beginning 
deposition. The specific weight at 25°C. is: 1.4022; at 50° C.:: 1.3688; 


ato? 1Gr 13359 Ata Gs: Ago = 1.4361—0.001366 ¢-+ 0.0000004 #2, 


V. 


Diethyl-Ethylbenzylmalonate: 
(C2H5)O . CO. C(CpHs) (C7H;). CO. O(CoHs). 


EB Maximum Pressure 7 Surface- ; Molecular 
a a = tension + Specific Surface- 
° . | : 
a. in mm. mer- in Erg. pro | gravity d energy v- in 
se cury of in Dynes wae - 2 
2 0-°C. i Erg. pro cm2, 
fo} ] 
—20.2 (2.174) (2898 . 4) (68.8) 1.086 (2775.0) 
Ome 1.241 1654.5 | 39.0 1.072 | 1586.7 
26 1.121 1494.9 35.2 1.052 1450.1 
| 45.5) 1.050 1399.9 32.9 1.035 1370.2 
66.6) 0.984 Sle 30.8 1.016 | 1298.7 
86.7) 0.940 1253.4 | 29.4 | 1.001 1252.1 
106 0.901 1201.2 28.1 | 0.986 1208.8 
126 0.853 1136.8 | 26.6 | 0.971 | 1156.0 
146 | 0.805 1073.2 2m } 0.956 1102.2 
| 166 | 0.759 1011.9 23.6 0.941 1047.3 
| 184 | 0.690 920.3 | 21.4 0.927 959.2 
206.5) 0.637 849.5 | 19.7 0.911 893.3 


Molecular weight: 278.18. | Radius of the Capillar tube: 0.04803 cm. 
Depth: 0.1 mm. 
Under 12 mm. pressure, the substance boils constantly at 189° C.; 


at — 79° C. the liquid becomes a feebly opalescent glass. Already at 
— 20° C. the viscosity is enormous, and at 0? C. again very great. 
The grow of the gas-bubbles at 0° C. lasted about 40 seconds. The 


specific gravity at 25°C. is: Ayo —HOpa ry at o0m Gor leOs22 ator Ges 
1.0098. At ¢° C. in general: A4o = 1.0725 — 0.000746 t—0.0000012 ¢’. 


VI. 
Dimethyltartrate: (CH3)0.CO.CH(OH)CH(OH).CO.O(CH3). 

| & . Maximum Pressure 7 Surface- eer Molecular 
| os ie ae ae | tension PECMIC Surface- 
| a. |in mm. mer-| _ in Erg. pro | gravity dy. | energy # in 
| =~ aye | in Dynes cm? Erg. pro cm? 

45° 1.490 1986.6 43.2 1.306 1144.6 
| 70.7 1.405 1873.1 40.7 1.281 1092.2 

90.7) 1.340 1786.5 38.8 1.261 1052.2 

116.2) 1.255 1673.2 36.3 1235 998.2 
135.5 1.200 1599.5 34.7 1:216 964.1 
159.6 1.046 1395.0 o2em Vai key 920.7 
"190 | 0.974 1299.2 30.4 sila 876.1 
| 210.3 0.929 1238.5 28.9 1.131 842.7 


| Molecular weight: 178.08. Radius of the Capillary tube: 0.04439 cm.; 
in the observations indicated with *, it was: 
0.04803 cm. 

Depth: 0.1 mm. 


The compound boils under 12 mm. pressure, at 180° C. constantly ; at 
—79°? C. it becomes a glass, which crystallizes with extreme slowness; | 


the solid substance melts at + 48° C. Even at 25° C. the ether is so 
viscous, that no reliable measurements were possible. 


z VII. 
Diethyltartrate : = 
(C,Hs)O. CO. CH(OH). CH(OH). CO. O(C2Hs). 
E f Maximum Pressure Surface- Specifi Molecular 
ae |e ————e tension , Beane Surface- 
ein mm. mer-| _ in Erg. pro | gravity d,, | energy » in 
a cy | in Dynes cm?, Erg. pro cm?. 
25° role 1755.5 37.6 1.210 1155.4 
45.3 1.241 1654.4 35.4 1.191 1099.3 
74.3) 1.134 1512.0 | aoe) 1.164 1018.5 
91.1 1.082 | 1443.0 | 30.8 1.147 980.8 
110.1) 1.024 I) 136429) 9) 29.1 1.129 936.5 
134.7) 0.948 1263.8 26.9 1.105 878.2 
| 150.1] 0.899 | 1199.4 | 25.5 1.091 839.6 
| 160.3 0.872 | IG 24.7 1.081 818.2 
| 192.7| 0.765 1019.9 22.0 1.050 743.1 
212.7) 0.716 955.9 20.2 1.032 690.2 
Molecular weight: 206.11. Radius of the Capillary tube: 0.04352 cm. 
Depth: 0.1 mm. 


Under circa 16 mm. pressure, the boilingpoint is 166.5 C. At —79° 

the liquid becomes glassy, and crystallizes very slowly at —20° C.: 

| only after 5 or 6 hours all has got crystalline. The meltingpoint is 

15° C, At 0° and lower temperatures the liquid is too viscous, to 
make reliable measurements possible. 


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400 


VIII. 
ortho-Nitro-Anisol : Cs . . CgHy. re 
( 


al 
| Ee | Maximum Pressure Surface- " Molecular 
ae | aa es — tension x Specific Surface- 
& | 01a 
0? 1.613 | 2150.4 50.8 e273 1237.6 
25.4 5S | 2048.8 48.4 1.247 | 1195.4 
44.9) 1.480 1973.8 46.6 1.227 1165.1 
70.1) 1.390 | 1853.0 43.7 1.202 1106.1 
85.3 1.340 1786.4 42.1 1.187 1074.6 
117 1.227 1635.8 38.4 1.156 997.6 
138.2) 1.160 1546.5 36.3 1.135 947.3 
| 156 1.109 | 1478.2 34.7 1.118 921.8 
| 172 1.043 | 1390.8 | 32.6 1.102 874.4 
191.5 0.968 1290.5 | 30.2 1.083 819.4 
| A 0.850 S350 e ss) 26.5 | 1.062 728.8 
—— a —- - -—— — = | — — — — 
Molecular weight: 153.07. Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 
The substance boils constantly at 272’ C.; at 20° it solidifies, 


and melts at + 10° C. Above 165° C. a slow decomposition begins. 
The specific weight at 25° C. is: Ayo — 124712" at o0Rn CG. al 22s mat 


75° C:: 1.1970: at ¢ generally: A4o= 1.2732—0.001052 t-+ 0.00000048 #2. 


IX. 
Methylsalicylate: C,;H,(OH).CO.OCH3 . 
ie ee (1) (2) 
vo | 4 
5 ' Maximum Pressure Surface- 4 Molecular 
eg | = = tension Specific Surface- 
Bs | in mm. mer- | in Erg. pro | gravity d,, | energy ” in 
= cury of in Dynes cm?2. Erg. pro cm2. 
(een SPP 
—19:8| 1.518 2023.8 44.2 1.220 1102.9 
0.3 1.436 1914.8 41.8 1.202 | 1053.4 
gee Sie 1829.0 39.1 1.179 998.1 
“45 1.303 1737.2 | Silo! 1.158 956.4 
Rr aewll 1.193 1590.1 | 33.9 1.128 | 891.7 
* 94 | 1.124 1498 2 31.9 1.110 | 848.3 
114.5) 1.031 1374 2 29.8 1.092 | 801.2 
13522 0.968 1290.5 27.9 1.073 758.4 
| 160.5 0.867 1155.9 24.9 1.050 | 686.7 
192.9 0.760 1013.7 21.8 1021-1) ) seieke 
212.2 0.696 928.1 19.8 1.003 | 562.9 


| Molecular weight: 152.06. Radius of the Capillary tube: 0.04439 cm.; 
in the observations, indicated by *, it was 
0.04352 cm. 
Depth: 0.1 mm. 


The substance boils at 217.°6 C. constantly; it can be undercooled 
| as far as —50° C, and crystallizes to a solid mass, which melts at 
| —16° C. At the boilingpoint z is: 19.3 Erg. pro cm?. The density at 
| 25° C. is: dyo = 1.1787; at 50° C.: 1.1541; at 75° Ce l28opAtee Cr 


Ayo = 1.2023—0.000924 ¢ —0.0000008 ¢. 


401 


X. 


Ethylsalicylate: C;H,(OH) .CO.O(C,Hs) . 
(1) (2) 


lars ; | 
ety Maximum Pressure H | Surface- : _ Molecular 
| BS tension | SITES Surface- 
oe ‘in mm. mer-) | | in Erg. pro | gravity dao | energy » in 
E-= | cury of | in Dynes | aa Erg. pro cm?. 
| (1 (C, | 
— ——st = — _ = — — 
0° 1.346 1794.5 39.1 1.154 
* 25 1.275 | 1700.4 36.3 180, Were 
e451} 1.206 1608.5 34.3 1.110 | 966.7 
|; a4. 1) 1.110 | 1479.8 SHES) 1.082 903.0 
\* 94.3] 1.047 | 1395.9 29.7 1.063 | 861.6 
} 115.1) 0.963 | 1284.1 27.8 1.043 816.7 
135.2} 0.906 | 1207.4 26.1 1.024 716.2 
159.8; 0.828 | 1103.8 23.8 1.001 118.6 
193 OM7123)) |) © 96452") 2087 0.980 633.9 
| 212.5 0.669 892.1 | 19.1 | 0.962 592.9 
Molecular weight: 166.08. Radius of the Capillary tube: 0.0 ‘439 cm. 
in the observations, indicated with * it was: 
0.04352 cm. 
Depth: 0.1 mm 
The substance boils at 231.°2 C. constantly; at —20° C. it solidifies 


and melts at ca. —10° C. At the boilingpoint y is 17.6 Erg pro cm?. 
The specific weight at 25° C is: 1.1298; at 50? C. : 1.1053; at 75° C.:1.0806. | 
At ¢@ it is calculated from: d4o = 1.1541—0.000968 ¢ -—0.00000016 7. | 


XI. 
Phenylsalicylate (Salol): C;H,;(OH) .CO.O(C Hs). | 
(1 
| = _ | Maximum Pressure Z | Surface- | } WeMolccnlartl| 
hy —————— | tension z Specific | Surface- | 
&. |in mm. mer-| | in Erg pro | gravity d,. | energy 4 in | 
(ES cury of in Dynes 2 [aSean ey ac) 2 | 
J 2, Erg. 4 
oe oc | | cm | rg. pro cm 
|—20-1| (2.613) (3482.8) | (76.5) 1.221 (2396.4) | 
0 | 1.571 | 2095.1 45.7 | 1.202 1446.7 | 
725) 1.485 1980.6 | 43.2 1.179 1385.2 
| 45 1.419 S925 3 5 41.2 | 1.160 1305.1 
TESS | 1035 EAT agk | 38.7 1.136 1272.0- | 
fe O0st) "4.272 © "|| ¥ 1605.8 36:8: 9/1120 122th tee} 
116 1.193 1590.4 34.5 1.098 1160.0 
| 135 1.132 | 1509.3 | 32.7 1.078 1130.3 
S16085) 0.971 | 1295.0 30.3 | 1.055 1046.3 
*189.8} 0.890 HTSO=i ee 27.7 1.026 974.5 
\*211.6 0.846 1128.5 | 26.3 1.006 637.5 
Molecular weight: 214.08. Radius of the Capillary tube: 0.04439 cm.; 
in the observations, indicated with * it was : 
0.04803 cm | 
Depth: 0.1 mm. 


Under 12 mm. pressure, the salol boils at 173° C.; at —33° C. it 
crystallizes spontaneously, and melts at +42? C. It can be under- 
cooled to a very high degree, and possesses a small velocity of crys- 
tallisation. At 35 C. the specific gravity is: 1 1697; at 50 C.: 1.1553; 
ator 11330 


402 


Some other derivatives of aromatic phenoles: Anzsol, Phenetol, 
Anethol, Guajacol, Resorcine-Mono-, and Dimethylethers; Hydrochinon- 
Dimethylether have been described before by the first of us). The 
temperature-coefficients of these compounds are however also reviewed 
in the present communication, because they were not mentioned in 
the one referred to. (Vid. also the preceding communications.) 
Molecular Surface energy 


in Erg pro cm?. Fig. 3. 


7220 
7190 
1160 


1130 


530 oe 
=20° O° 20° 40° 60° 80° 100° 120° 140°160" 180" 200° 220° Semperalure 


1) F, M. Jarcer, These Proc., Comm. I. (1914) p. 354 seq. 


403 


XII, 


Methyl-Cinnamylate: CjH/,.CH:CH.CO.O(CH,). 


| 


5 , Maximum Pressure H | Syurface- | - | Molecular 
ise = 3 —_| tension x Specific Surface- 
a jin mm. mer- in Erg. pro | gravity d,, energy » in 
eo cury of in Dynes | em?, | : Erg. pro cm?. 
Ee O2NE: | | | 
45, HeS20r ee LIL S le | 38-1 AN | 7 1062 Ne anOs.2 
71 1.230 1639.8 | 35.8 1.038 } 1038.1 | 
90.6) 1.166 1554.5 | 33/69 | 1.020 | 994.5 | 
116.2) 1.092 1455.2 Madi | 0.997 944.2 
135.4) 1.024 136552555) 29.7 0.980 894.9 | 

*159.7} 0.868 ) sea | Palle! 0.958 | 829.0 | 

*190.5) 0.777 | 1035.9 | 24.2 | 0.930 | 155) )lenmn| 

*210.9 0.712 949.4 | Doel | 0.911 | 699.1 


Molecular weight : 162.08. Radius of the Capillary tube : 0.04439 cm.; 
* in the observations, indicated by * it was: 
0.04803 cm. 
Depth: 0.1 mm. 


point ~ is: 18.6 Erg. pro cm?. The specific gravity at 35°C. is: 
@4o = 1.0700; at 50° C.: 1.0573 at 75° C.: 1.0340. 


| 

| 

| 

The ether boils at 253.°5 C., and melts at 36.°5 C. At the boiling- | 
| 


§ 3. Values of the Temperature-coefficients of the molecular 
surface-energy & of the studied compounds. 


Amylacetate. | Diethyl-Ozalate. 
Oe. Ou . 
Temperature-interval: ae in Erg: | Temperature-interval: ae in Erg: 
i | at 
between — 70°? and — 21° 2,59 | between — 20° and 0° 1,8 
— 219 and -- 662 -2)14 0°? and 66° 2,02 
66° and 106? 2,03 66° and 106° 2,2 
106° and 148° 1,73 106° and 146°? 2,3 
146° and 184° 3,6 


| Above 146? a decomposition seems 
slowly to set in. 


Diethyvlmalonate. Diethylbromomalonate. 

between — 20? and + 171° 2,52 | between — 21° and 0° 3,20 
} 0°? and 26° 3,08 

| 26° and 46° 2,67 

| 46> and 67° 2,04 

67° and 86° 1,75 

86° and 106° 1,63 

106° and 126° 1,35 


126° and 146° 1,23 


404 


Diethyl-Ethylbensylmalonate. 


Ou 
Temperature-interval: - in Erg: 
t 


between —20° and 0° cannot be deter- 


mined indepen- 
dently of the vis- 
cosity. 
OO wae 5,2 
AN oy (HO 3,7 
66° ,, 106° 2,25 
106gm,, 126° 2,6 
1262" 5, 146° 2 
1462 wl OGSe- 2,15 
166° ,, 206° 3,85 


| 


Above 166° a slow decomposition begins | 
to make itself perceptible. 


o-Nitroanisol. 


between 0° and 45°? 1,61 
45°, 172°? 2,29 | 
Wize loos 2,82 
egy ee Pye) 4,45 


Above 170°? a gradual decomposition | 
sets in, which proceeds very slowly. 


Ethylsalicylate. 
between 0° and 212° 2,23 
Methylcinnamylate. 
between 45° and 210°,9 2,44 
Phenetol. | 
between —12° and 0° 2,0 
0? , 74°,3 2,29 
74°, 160° 2,13 
The curve is almost a straight line, | 
Om 
with sama 
Ot 
Guajacol. 
between 26° and 146° 2,17 
1462, 2062 2,66 


Dimethyltartrate. 
Ou 
Temperature-interval: x in Erg 
t 
between 45° and 117° 2,08 
117°, 160° 1,71 
160° ,, 210° 1,53 
Diethyltartrate. 
between 25° and 74°,3 2,15 
pen Pile 2,35 
Methylsalicylate. 
2,30 


between —19,°8 and 212° 


Phenylsalicylate. (Salol). 


| between —20° and 211°,6 2,43 
Anisol. 
| between —21° and -+45° 1,88 
B52 91° 2,14 
Co ole 2,63 
Anethol. 
between 24°,7 and 75°,1 2,53 
15 eo 2,25 


Resorcine-Monomethylether. 
between —20° and O° cannot be deter- 


mined indepen- 
dently of the vis- 
cosity. 
QO 5 Base 4,3 
26° OS 2,45 
46° ,, 184° 1,82 
184° ,, 206° 2,97 
Above 184° a decomposition sets in 


slowly. 


405 


Resorcine-Dimethylether. Hydrochinon-Dimethylether. 
Ou Ou 
Temperature-interval: va in Erg: | Temperature-interval: x in Erg: 
t | OF 
between —22° and U° 2,83 between 66° and 106° 2,11 
D2 Vo Poe 2,2 | 106° ,, 166° 2,46 
166° ,, 206° 2,88 


Up to 166°, this -tcurve coincides 
| practically with that of guajacol and of 
resorcine-dimethylether. 


Pyridine. | z-Picoline. 
between —79° and —20° 1,79 between —70° and — 20°77 2,83 
—20° , +25° 2,04 —20°,7 , +126° 2,02 
25o re 92° 1,60 
Chinoline. | 
between —21° and +45°,2 1,92 
45°, 115° 2,10 
5 2302 2,33 


§ 5. Also tor these substances one can state, that a decom- 

position of the compound causes an extraordinarily rapid decrease 
age Ou 

of the values for x or « with inereasing temperature : a becomes 
much larger in such eases with rising temperature. Furthermore it 
can be seen from the cases of salo/, diethylbenzylmalonate, resorcine- 
monomethylether, etc., that an extraordinarily great viscosity of the 
liquid can appreciably diminish the accuracy of the measurements ; 
however the case of dimethyltartrate on the contrary proves, that 
sometimes reliable results can be obtained, even with very high 
values of the internal friction. 


Groningen, June 1914. Laboratory Inorganic Chemistry 
of the University. 


Chemistry. — “Vhe Temperature-coefficients of the free Surface- 
energy of Liquids, at Temperatures from —80° to 1650° C.; 
V. Measurements of homologous Aromatic Hydrocarbons and 
some of their Halogenderivatives’. By Prof. Dr. F. M. Janerr. 
(Communicated by Prof. P. van RompBvurGu.) 


§ 1. In order to answer also the question of an eventual depend- 
ence between the chemical constitution of liqnids and the values 
of their free surface-energy and of its temperature-coefficient, in 

27 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


406 


this communication the results of the measurements are recorded, 
made with a series of homologous hydrocarbons and some of their 
halogen-derivatives. With respect to the methods of purification, the 
determination of the specific gravities, and the significance of the 
diagrams, we can refer to the previous communications. 

This series includes the following terms : 


Benzene; Toluene; para-Xylene; Mesitylene; Pseudocumene; Tri- 
i y 

phenylmethane; Chlorobenzene; Bromobenzene ; meta-Dichlorobenzene ; 

yara-Eluorobromobenzene; meta-Eliorotoluene; and para-Chlorotoluene. 

l 


For the purpose of comparison with benzene, also Cyclohevane 
was taken into account here; the data relating to benzene were’ 
already published in a former paper‘), but are repeated here once 
more for comparison with the other hydrocarbons. The obtained 
results are put together in tables, in the ordinary way. 


§ 2. Aromatic Hydrocarbons and some Halogenderivatives. 


it 
Cyclohexane: CgHjo. 

= ; Maximum Pressure H Surface- ee Molecular | 

a = _ tension % pecific Surface- | 

Be in mm. mer-| in Erg. pro gravity d,, | energy in 
| ca euro in Dynes | cm? Erg. pro cm?. 
he U c : | eee \ as: s. | 
| | | a Fes | 
Ha? 0.830 | 1106.8 28.3 0.788 636.7 
| 19 0.785 | 1046.5 26.7 0.778 605.9 
124.6 | 0.755 1007.6 25.7 OR Seo 

40 0.682 909.2 23m 0.768 BPA Pa = | 
| 58 0.601 | 801.2 20.3 0.744 474.6 | 
| 70 0.548 730.6 18.4 0.732 434.9 | 
| 80 0.504 | 671.6 16.9 0.723 402.7 


Molecular weight: 84.1. Radius of the Capillary tube: 0.05240 cm. 
Depth: 0.1 mm. 


The liquid boils constantly at 80.°7 C.; at this temperature the value 
of x is: 167 Erg. pro cm®. Jt solidifies at 10 C.; the crystals melt at 
+8 C. The specific gravity at 25° C. is. 0.7733; at 35° C.: 0.7645; " | 
at 502707515 At tame, d4> = 0.7958—0.000913 ¢ + 0.00000053 #7, | 


1!) FB. M. Jaccer and M. J. Smit; F. M. Jazarr and J. Kann; F. M. JAEGER, 
these Proc., Gemm. I, II, IV. (1914; 


407 


II. 


Benzene: CoHg. 


| E Maximum Pressure Z | Surface- idee Molccula®. | 
SS — _| tension x peeie Surface- 

|. jin mm. mer-) _ in Erg. pro | gravity d,, | energy » in 

ao CaS | in Dynes | cm?. | Erg. pro cm?. 

=a ———————— = = = = 
5.4 1.077 1436.7 30.9 0.895 607.7 
9.5 1.055 1406.5 30.2 0.889 596.6 
owl 0.969 1291.9 | 27.7 | 0.873 553.8 
35 0.920 1226.5 26.3 0.862 530.3 
55 0.836 1114.6 |} 23.8 0.841 487.8 
714.6 0.757 1009.2 21.6 0.817 451.4 


Molecular weight: 78.05. Radius of the Capillary tube: 0.04385 cm. 
Depth: 0.1 mm. 


The compound was already formerly described !), and is here only 
mentioned for purpose of comparison. The boilingpoint is 80.5 C.; 
at this us ty DoE x is: 20.7 Erg. pro cm?. 


1) JAEGER, These Proceedings, Comm. I. (1914). 


Tin 


Toluene: CH,. C,H;. 


5 : Maximum Pressure /1 _ Surface- eee Molecular | 
oe = tension 7 Preemie Surface- | 
vo =) . 
a jin mm. mer- in Erg. pro | gravity d,, | energy # in | 
ES cury of in Dynes | em2 Ao 2 | 
& 0°C. Erg. pro cm? 
| | 
I—71 | 1.385 1946.5 | 43.7 | 0.956 918.1 
—21 | 1.090 Ip 45325 7 34.3 0.905 | 747.6 | 
Om 1.006 1340.8 31.6 0.884 | 699.5 | 
26 0.906 1207.16) 5} 28.4 0.860 640.3 
46 0.831 1107.6 26.0 0.841 595.0 | 
66.6 0.756 | 1007.7 | 23.6 0.823 547.9 
| 86.5 0.693 924.4 21.6 0.803 509.7 
| 106 0.637 849.5 19.8 0.783 475.2 
| | 


INoteeurar Weishe: 92. 06. Radius of the Capillary tube: 0.04803 cm. 
Depth: 0.1 mm. 


The commercial toluene appeared always to manifest a turbidity 
of the liquid at — 22° and —79° C.; a solid substance in little quan- 
tities separated at the walls of the tube. The here used toluene there- 
fore was especially prepared by distillation of sodium phenylacetate; 
it was dried by means of phosphorpentoxide, and boils at 109.°4 C, 
Down to —20°C. it remains perfectly clear; at — 79° C. it shows, as 
e.g other hydrocarbons (pseudocumene) do, a slight turbidity, At ‘the 
peer z is ee es pro cm?, 


PHT fi 


para-Xylene: (CH,) .CgH,. 
(1) 


(CH3) . 
(4) 


| 


E 7 | Maximum Pressure /I Surface- 
go tension 
a. in mm. mer- ' in Erg. pro | 
e cury of in Dynes cm?2. 
= OFIG: 

a_| 
Zoe 0.928 1236.7 29.1 
45.9 0.853 1137.2 26.7 
66 0.774 1031.9 24.2 
86.5 0.709 945.2 22.1 
106 0.648 863.9 20.1 
126 | 0.597 7194.6 18.5 


Molecular weight: 106.08. Radius 


Depth: 0.1 mm. 


The substance boils at 136.°2 C. 
point z is about 181 Erg. pro cm?, 


Specific 


gravity d4o 


Molecular 
Surface- 
energy » in 
Erg. pro cm’, 


of the Capillary tube: 0.04803 em. 


and melts at 15°C. Atthe boiling 
At 20° the density is Ayo = 0.8611. 


V. 
Mesitylene: (C/Z,);.CgH,. (1-3-5-). 
= ‘ Maximum Pressure JI Surface- : Molecular 
we tension ~ Specific Surface- 
a in ua. mee ve | in Erg. Pro | gravity d4o energy in 
Thien y o in Dynes em?, Erg. pro cm?. 
coal | DXC. | 
= | — . — = ————— ee 
20-8 1.141 ! 1521.1 32.6 0.897 | 853.2 
hy OL. | 1.061 1415.4 30.3 | 0.880 803.2 
25.5 0.972 1296.0 iles| 0.859 746.2 
45.2| 0.907 1208.7 25.8 0.843 703.8 
140i 0.807 1075.4 | 22.9 0.818 637.3 
91.3 0.755 1006.4 21.4 0.804 602.5 
110 0.700 933.0 19.8 0.788 565.0 
134.5 0.631 841.0 17.8 0.768 516.7 
150.5 0.585 Ula. | 16.5 0.754 484.8 
160.5, 0.562 749.3 | 15.8 0.741 469.7 
| 


| 


Molecular weight: 120.1. 
Depth: 01 mm. 


The compound boils at 162.°8 C. constantly. At —46° C. it soli- 


difies to an aggregate of long, silky needles. 


Radius of the Capillary tube: 0.04352 cm. 


VL. 
Pseudocumene: (C//3), . CgH; (1-2-4-). 
lia l Tr i z 
| 5 _| Maximum Pressure H | Surface- | cee le Molecular 
ig — —_ = | tension x pecilic | Surface- | 
rae ‘in mm. mer-) | in Erg. pro gravity d, | energy in | 
e= cury of in Dynes | cm. ‘ Erg. pro cm?. 
= 0G: | | 
= — 1 = = — ———— = SS SSS = 
Bo ee ag) aa 0.910 | 883.9 
| 0 1.031 | Is74eiy |) 3274 0.893 850.5 
26 0.953 1270.1 29.9 0.871 798 .0 
46 | 0.890 1186.4 27.9 0.855 153.9 
66.5 0.828 1103.5 25.9 0.839 708.8 
86.5, 0.768 1024.4 24.0 0.823 665.2 
105 0.725 966.1 | 22.6 0.807 634.7 
125 0.656 | 874.5 20.4 0.792 | 580.1 
145.9, 0.600 799.5 18.6 0.776 536.2 
; 166 0.525 699.6 | 16.2 0.760 473.5 


Molecular weight: 120.1. Radius of the Capillary tube : 0.04803 cm. 
Depth: 0.1 mm. 


The substance boils at 168.°5 C. constantly. It solidifies at —79° C.; 
the meltingpoint is about —60° C. At the boilingpoint the value of 
z is 15.8 Erg. pro cm?. 


Molecular Surface- 
energy in Erg pro c m2. 
960 


450 
-S0°-60°-Y0°-20° O° 20° 40° 60° 80° 700° 720° 140° 760° 780° 


Fig. 1. 


Temperature. 


Triphenylmethane: CH (C,H;);. 


2) | 

5 4 | Maximum Pressure /I Surface- 

ae _—_— | tension x 

| ae in mm. met : | in Erg. pro 
E--= | cury of in Dynes cm2, 

[ec | 0°C. 

—— = = SSS = SSS a 

| 138.4] 1.074 145254 pl) ones 

| 156 1.044 1391.9 32.8 

| 7p 0.999 | 1332.5 31.3 

; ee  Wesia) 1211.9 28.4 

0.833 1110.5 26.0 


Specifi Molecular 
peeric Surface- | 
gravity d45 energy » in | 
Erg. pro cm? 
0.984 1330.5 
0.971 1302.6 
0.959 1257.1 
0.942 1154.4 
0.928 1067.4 


, Molecular weight: 244.11. Radium of the Capillary tube’: 0.04803 cm. 
Depth: 0.1 mm. 

The meltingpoint of the compound is 92° C.; it is hardly possible 
to keep it in undercooled condition. Above 165° C. a slow decom- 
position begins; finally the liquid is coloured brown. The specific 
gravity 40 is at 95° C.: 1,017; at 100°: 1,013; at 125° C.: 0,994; at 


150° C.: 0,975; it was determined by means of the hydrostatic balance. 
Ate ayo = 1,013 — 0,00076 (¢ — 100). 


VIII. 


Chlorobenzene: C,H, Cl. 


E Maximum Pressure H 
aU | 
So, | See 
a. jin mm. mer- 
Es cury of in Dynes 
om Ov 
o} 
—16 1.252 1668.8 
0 1.184 1578.3 
25 1.143 1524.5 
rao 1.099 1465.5 
| 50 | 0.980 1306.6 
70.5) 0.893 1190.2 
| 90 | 0.805 1079.0 
\*102 0.807 | 1075.4 
Stas 0.751 1001.8 
= 12255 0.717 955.9 


| 


Surface- 

| tension x 
in Erg. pro 

cm?, 


Specific 
gravity d 40 


Molecular 

Surface- 
energy in 
Erg. pro cm?, 


es 
| Palio 


So 
HUW CAMCCO 


is) 
oO 


144 
128 
101 
090 
-078 
051 
029 
O16 
-003 
-995 


as ee a 


completely crystallized. 


The compound boils at 131? C. 


Molecular weight: 112.5). Radius of the Capillary 
with the observations, indicated by *, R 
was 0.04352 cm.; with those: **, it was: 
0.04408 cm. 
Depth: 0.1 mm. 


tube: 0.04638 cm.; 


constantly; at — 34.°5 C. it is 


41] 


Ix. 


Bromobenzene: C,H, Br. 


= : Maximum Pressure | Surface- | 
aS — : tension i | 
26 in mm. alee | in Erg 
‘= | mercury 0 in Dynes ro cm?. 
& | One: ae 
° | 
—17.5 1.394 | 1858.6 42.2 
ee 1.309 |) 1746-4 | 39.6 
~25 1.267 | 1698.5 | 36.5 
*35.6 1.229 | 1638.5 | SHge 
*49.8 1.172 156255 33.5 
71.5 1.032 ISTEEO || 31.0 
90.5) 0.953 | 1270.5 28.5 
125.5) (0.875 1167.3 24.5 
pal53 0.758 LOWER) 21.1 


Depth : 0.1 mm. 
The compound boils constantly at 154° C. 


X. 


Molecular weight: 156.96. Radius of the Capillary tube: 0.04638 cm.; in 
the observations, indicated by * R was: 
0.04408; in those by **, it was: 0.04352 cm. 


meta-Dichlorobenzene: C,H, Cl, (1-3-). 


The boilingpoint is at 172.55 C. constant; the liquid can be under- 
At 


= Maximum Pressure H | Surface- Molecular | 
= a | tension x Surface- 
ie in mm. | in Erg enerey 2 
| —-= mercury of | in Dynes | pro cm2. in Erg 
DC. | pro cm?. 
—22 1.433 1910.3 41.6 956.8 
0 1.328 1770.6 38.5 895.9 
25 1.230 1640.0 35.6 840.0 
44.9 1.156 1540.9 33.4 797.9 
irl 1.061 1414.7 30.6 Ti2.2 
| 90.7 0.993 13246 =| 28.6 700.2 
| 116.4 0.912 1216.5 | 26.2 651.5 
| 136 0.858 1144.4 24.6 619.0 
“160 0.737 982.7 22.8 582.4 
PIE dl ee é a ee 
| Molecular weight: 146.93. Radius of the Capillary tube: 0.04439 cm.; 
in the observation, indicated with *, the 
radius was: 0.04803 cm. 
Depth: 0.1 mm. 


cooled to a high degree, but once solidified, it melts at —19° C. 


the boilingpoint ~ is: 22.2Erg pro cm?. The specific gravity at 25°C. 
is: 1.2824; at 50°C.: 1.2543; at 75° C.: 1.2253; at f C.: 1.3096—0.00107 ¢ 


| —0.00000072 f. 


Molecular | 
Surface- | 
energy » 
in Erg 
pro cm?. 


} 


Molecular Surface- 


energy in Erg per c.m?*. 


412 


450 2 — Temperature. 
-40°20° 6° 20° 4b° 60° EI? 100° 120° 440° 60" 18D” 
Fig. 2. 
XI. 
| para-Fluorobromobenzene: C,H,. /. Br (1-4-). 
_——S ee ES : : ey 
£ | Maximum Pressure H | Surface- Molecular 
| ee ian Specific Surface- 
| &. jin mm. mer- | in Erg. pro | gravity d@,,| energy v in 
ears cury of in Dynes cm2, | Erg. pro cm?. 
= OG: | 
eines 1707.8 398 | 1.654 890.2 
0 1.198 1597.2 37.2 1.626 841.5 
25.5 1.106 1474.1 34.3 1.590 787.6 
45.3 1.031 1374.1 31.9 1561 741.6 
710 0.953 1270.1 29.4 1522 695.1 
84.7| 0.906 1207.6 27.9 1.504 663.8 
Hedi 0.810 1079.9 24.8 1.460 602.8 
| 138 | 0.734 978.6 22.4 1.436 550.5 
Molecular weight: 174.95. Radius of the Capillary tube: 0.04803 cm. 
Depth 0.1 mm. 


The boilingpoint is constant at 150° C.; the value of x there is: 
21.2 Erg. pro cm’. The specific gravity at 25° C. is: Ayo = 1.5998; 


| tat 50Gs 15538; atwiocn Ga M5147) eAb eaiteis. @4o = 1.6257 —0.00135 
| t—0.00000168 #2. 


oats 9 


413 
XU. 
meta-Fluorotoluene: CH,.Cs,H,.F . | 
(3) | 
; : i Rests | 
— Maximum Pressure | Surface- Fal Molecular 
ig = 2 | tension ~ Specific | Surface- 
| &e jin mm. mer-| — | in Erg. pro | gravity d A energy / in 
| & | cury of in Dynes | cm?. oat Erg. pro cm2., 
is eed | | 
Ae oe as _ aE en | 
ie || Bessy 1782.5 42 | 1.097 909.0 
—20.5 1.090 1453.3 34.2 1.041 764.7 
0 1.006 1340.9 31.5 1.021 TNS: 
25.4 0,906 1207.9 28.3 0,994 652.6 
, 45.3 0.839 1118.5 26.2 0.973 612.8 
| 70.2 0.760 1021.2 23.8 | 0.947 566.8 
84.9 0.721 961.9 22.4 | 0.932 539.2 


Erg. pro cm? 


Molecular weight: 110.06. 


Dept 


h: 0.1 mm. 


Radius of the Capillary tube: 0.04803 cm. 


The boilingpoint of the substance is 114°.5 C.; 7 is there: 20.2 
The density at 25° C. is: 


d4> 1059942 o0P G: 


0.9680; at 75°C.: 0.9420. At © it is calculated from: d4o= 1.0206— 
—0,00106 ¢ + 0.00000016 ?. 


Molecular weight: 126.51. 


Radius of the Capillary tube: 0.04439 cm.; 


in the observation, indicated by *, it was: 
0.04803 c.m. 
Depth: 0.1 mm. 


The substance boils constantly at 162.5 C.; it solidifies at —22°C., 
| and melts at +7.°5 C. At the boilingpoint z is 20.1 Erg. pro cm?. 


XII. 
para-Chlorotoluene: CH3;.CgH,Cl . 
: (4) 
£ | Maximum Pressure H Surfaces Malecutar 
Se = — = tension SERENE | Surface- 
a. |inmm.mer-| _ | in Erg. pro | gravity d,| energy “in | 
| &= | cury of in Dynes | em?2, " *lErg. pro cm?, 
= (HG: 
25) 1.137 1515.8 32.9 1.065 795.0 
44.7 1.059 1410.2 30.6 1.045 748.8 
71 0.959 1279.6 Plot 1.018 689.8 
90.2 | 0.895 1193.2 25.8 0.999 650.6 
| 116.1]. 0.813 1083.9 23.4 0.973 600.6 
135.7 0.760 1013.8 21.8 0.953 567.3 
*160 0.653 870.3 20.2 0.928 535.1 


414 


Molecular Surface-energy 
in Erg pro cm?. 


7020 
290 
960 
930 
200 


S70 


450 
-80°60-40"-20° O° 20° 40° 60° 80° 100° 120 ryo'réo' 760" ‘Temperature 


Fig. 3. 


§ 8. Values of the Temperature-coefficients of the molecular Sur- 
Fface-energie & of the liquids here studied. 


Cyclohexane. | Benzene. 
; Ou. . Ou. 
Temperature-interval: a in Erg: Temperature-interval: ae in Erg: 
Ot 
between 9 and 80° Be between 5°,4 and 25°,1 2,73 
This value is remarkably great; the 25 » 0D 2,20 
curve is almost a straight line however. 55 » 14,6 1,85 
Toluene. para-Xylene. 
between —71°? and —21° 3,40 between 25°,5 and 45° 2,53 
Ve 2 GAS 2,27 45286 2,43 
Gili 86,5 1,90 86 » 106 2,21 
86,5 , 109 1,76 106 7 126 1,71 


415 


Mesitylene. Pseudocumene. 
Temperature-interval: a in Erg: Temperature-interval: = in Erg: 
between —20°,8 and 0° 2,40 between —21° and 0° 1,60 

0 lO 2,20 QO 2 2,00 
15 » 110 2,06 20h an LAG 2,18 
110 POO 1,97 146, «166 3,0 
Triphenylmethane. Chlorobensene. 
between 138°,4 and 156°? 1.59 between —16° and +25° 2,20 
156 = algal 3.03 2 50 2,42 
gil ney! 4.46 SOE e122 2,60 
194 » iz 4.83 
Bromobengene. meta-Dichlorobengene. 
between —17,°5 and +125,°5 =.2,38 between —22° and 09° 2,79 
1:25)50n,, 153 2,53 O) =) 224) 2,23 
25 yo Anti 
Ol se 1,88 
WG si SS 1,64 
136, 160 1,51 
para-Fluorobromobenzene. meta-Fluorotoluene. 
between —21° and 0°? 2,41 between —71° and —20°,5 2,85 
OF} j 45 2,09 —20,5 , 0 2,49 
ey py Lily 1.97 On, 25,4 2,38 
lily EO) 2,49 25,45 45,3 1,99 
45,3 84,9 1,85 
para-Chlorotoluene. 
between 25° and 45° 2,33 
45 ay HL 2,23 
Tie wallG Lor | 
L1G, 160 1,49 


| 
Especially the last mentioned four cases prove once more very 


Ou 
strikingly the fact, that re cannot be considered as a constant, but 
r t 
that it is itself a function of temperature: in most cases in such a 
way, that it will decrease with increasing temperature. With ch/oro- 
and bromobenzene however evidently just the reverse happens. In the 
same way benzene, toluene, p-vrylene and mesitylene belong to the first 
group of substances, while the isomeric psewdocwmene manifests on 
A Caen a 
the contrary an increase of — with rising temperature. The devia- 
tions of the linear decline are so great and in most cases so system- 
atical, that they can by no means be accounted for by experimental 
ae MOBY Fas 
errors; the variability of F with the temperature must therefore 
° t 
be considered as an essential fact. 
Groningen, June 1914. Laboratory of Inorganic Chenustry 
of the University. 


416 


Chemistry. — “The Temperature-coéfficients of the free Surface- 
eneryy of Liquids, at Temperatures from — 80° to 1650°C: 
VI. General Remarks”. By Prof. Dr. F. M. Janexr. (Commu- 
nicated by Prof P. RompBuren). 

§ 1. If we wish to use the results up to now obtained in the 
study of these more than seventy organic and about ten inorganic 
liquids, to draw some more general conclusions, the following remarks 
in this respect may find a place here. 

In the first place it is proved once more, that the free surface- 
also in the peculiar case of the electrolytically 
conducting, molten salts studied at very high temperatures, — always 
decreases with increasing temperature. This fact, an exception to 
which also within the temperature-interval hitherto investigated — 
has never been stated, must be esteemed in every respect quite in 
concordance with the views about the origin of such surface- 
tensions. It is immediately connected with the other fact, that 
a decrease of the molecular surface-layer must be accompanied 
by a heat-evolution, an increase of that layer however with a heat- 


energy of liquids, 


absorption, if the temperature is to remain constant. Furthermore 
this gradual diminution of % with increasing temperature is in full 
agreement with the continual levelling of the differences in properties 
between the liquid phase and its coexistent vapour, when the 
temperature is gradually rising: at the critical temperature the value 
of y must have become zero’). 

Of more importance for our purposes however are the following 
results : 

I. A linear dependence of y and ¢ appears in general noé to exist. 
1] The observations prove the possibility 
; of all the three imaginable principal spe- 
cies of y-é-curves: the type 1, with a 
concave shape towards the temperature- 
axis; the type 3 with a shape convex to 
that axis; and the rectilinear type 2. 
Besides there are found some rare cases 
of combinations of these three principal 
types. Characteristic for type N°. 1 is, 
that oh will inerease with rising tempe- 


at 


rature, while it decreases under those 


oO t 


circumstances on the curves of type 3; 


1) The critical temperatures of the studied liquids, are as far as known, in the 
diagrams indicated between ( ), behind the names of the different substances. 


417 


only in the case N°. 2 this quotient remains really constant. It is 
now of importance to draw attention to the faet, that in contradiction 
with the hitherto prevailing views, the presence of type 2 on one 
side, and of types 1 and 3 on the other side, appears to be in no 

: s : : du é 
clear connection with the absolute value of the quotient a nor with 
the absolute values of x or w themselves. 

Il. In agreement with the results of previous investigators, it 
appears to be possible, although only in some arbitrary way, to 
divide the studied liquids into fo principal groups, with respect to 

du 


the value of —. In the first group A belong all liquids, whose 
at : 


, du 
quotients = really are very near to Eérvés’ “constant”: 2,27 Erg 
a 
pro every degree Celsius. However it must be said here, that only 
a F. 
a mean value of = evidently can be considered in these cases, and 


only over a sparely extended temperature-interval; for, just as we 
already mentioned sub I, these liquids will by no means always 
show a linear dependence of y and ¢, corresponding to the type 
2, and therefore such a linear dependence may be supposed in most 
eases only for rather short parts of the curves in question. 

To this group A we can bring e.g.: a number of ethers, like 
Ethyl-Isobutyrate (2,15); Tsobutyl-Isobutyrate (2,18); Diethyl-Ovalate 
(2,26); Diethylmalonate (2,52); Diethyltartrate (2,35); Ethyl-Acety/o- 
acetate (2,19); further: Chloroform (2,06); Dimethylaniline (2,23); 
Phenetol (2,14); Anethol (2,25); Methylbenzoate (2,21); Ethylbenzoate 
(2,29); Methylsalicylate (2,30); Ethylsalicylate (2,23); Methylcinna- 
mylate (2,43); a-Picoline (2,02); ete. 

With most of these and analogous substances however, we can 
state a considerable increase of at /ower temperatures (type 3), and 

at 
for many of them a value in the vicinity of 2,27 may be accepted 
only within a very narrow range of temperatures, e.g. between 
25° and 80° C. 
45 ; du 

To the group £6 all liquids belong, whose quotients = show 
values appreciably lower than 2,27 Erg pro 1°C. To this group the 
following substances can be brought: Water (1,04); Ethylalcohol 
(0,94); Propylalcohol (1,10); Tsobutylaleohol (1,10); Acetone (1,6) ; 
Acetic Acid (1,3); Pyridine (1,6); ete. However with several of these 


418 


du, 
liquids the value ot ; increases much at the lower temperatures, 
at 


while to the other side many liquids of group A, which e. g. between 
Oe 
25° and 80°C. show rather normal values of vo will have abnor- 
mally low values for it at the higher temperatures. As far as the 
not numerous determinations of the specific gravities make a con- 
clusion possible in this respect, to this group 4 can be brought also 
the molten salts of the alkali-metals: Sodzmehloride (0,6), Potrssium- 
chloride (0,64); ete. Furthermore the hitherto observed dependence 
of x and ¢ for: Sodiumsulfate, Sodiummolybdate, Sodiumtungstate, 
Sodiumphosphate ; Potassiumbromide, Potassiumiodide,  Potassium- . 
phosphate, -molybdate, -tungstate ; Lithiumsulphate, Lithiummetaborate, 
Lithiummethasilicate ; ete. ete., -—— seems to prove, that also with 


Oe: 
these salts the values of 5 will appear to be remarkably small. 
Ot = 


§ 2. The prevailable opinion is, that the liquids of the group B 
must differ from those of group A in this respect that they would 
be associated, while the liquids of group A would be normal ones. 
Regarding those liquids, which show an almost linear dependence 
of y% and ¢ (type 2), the “association-coefficient” x is then calculated 


3 
: 2,2 |2 
from the expression: «= \— 


Ow 
I(r) 
a linear dependence can not be supposed, several other formulae are 
proposed"). After what has been said, however, it can hardly be quite 
sure, that such a calculation of the degree of association can be 
thought of as a step in the good direction. For among the substances 
of group A the greater number are of a kind, whose «-t-curves 
belong to types 1 or 3; type 3 can be thought moreover again to 
be in so far in agreement with the postulations of the theory, that 


- while in the cases, where such 


here at least exists the possibility that the curve will approach 
to the axis asymptotically in the vicinity of the critical temperature. 
If now however the supposition were right, that a decrease of 


1) After vAN Der WAALS (Z. f. phys. 18. 716. (1894)) e. g., a relation of the 


: T \B 

form: wt = A{ 1 — —] , — in which B at the critical temperature should 
ot Vr 

have the value: 3/o, but im praxi appears to be: about 1,23, — would reproduce 


in many cases the dependence of y and / to a rather sufficient degree. 


419 


Ou 
the values for va indicated an augmenting degree of association, it 


would be very difficult to imagine, why the larger number of 


liquids just show u-teurves of the type 3: for from the gradual 
Ola suse : 
decrease of a with increasing temperature in these cases, we must 
; 2 


conclude, that the association of the liquid would increase for most 
liquids with a rise of temperature. But because by far the most 
dissociations are accompanied by a heat-absorption, the mentioned 
conclusion could surely be hardly put in concordance with the laws 
of the mobile equilibrium. With liquids, which will dissociate to a 
higher degree at higher temperatures, one had to expect on the 
contrary the progress of type L: water e.g. is such a liquid, showing 
a gradual dissociation of complex molecules into simpler ones at 
increasing temperatures, and the «-tcurve here really possesses ') 
the expected type 1. In the same way we observed some organic 
liquids (Diethyl-Ovalate; Ethyl-Propylacetyloacetate;  Propyl-, and 
Isobutyl-Cyanoacetates ; — 0-Toluidine; Resorcine- Monomethylether ; 
Hydrochinondimethylether ; a-Campholenic Acid; ete.), for which 
a gradual dissociation or decomposition at higher temperatures 
could be stated, and for those we found also a faster increase of 


Oye a 
a than before, as soon as the temperature of beginning decomposition 
t 


was surpassed. In opposition therewith is the case of acetic acid, where 
a gradually proceeding depolymerisation with increasing temperature 
has been quite doubtlessly proved, and where notwithstanding 


u 


0 
this fact, the value of va remains constant within very wide limits 


of temperature. *) 
These facts seem after my opinion to make it very dubious, if 


Ou 
the increase or decrease of a with varying temperature can be esteemed 
: ying 


mot: ‘ , : { 
1) From E6éryés’ observations one can deduce already immediately Pek 
t 


will increase with rising temperature in the case of water: he observes between 
3° C. and 40°C. a coefficient: 1,59; between 40°C. and 100° C.: 1,80; between 
100° ©. and 150° C.; 2,28; and between 150° and 210° C.; 227. 


®) Also this fact can be already de jiuced from Eérvés’ observations: between 


l 
91° and 107° GC. he finds for —:; 1,52; between 107° and 160° GC. also: 1,82; 


Ot 
between 160° and 280° C.; 1,38. 


420 
any longer to be connected directly with the degree of association 
of liquids? 
Son ae , On :; Mee 
§ 3. The variations of 5 must in the first instance be dependent 
t 


on the way, in which the specific heat ¢ of a liquid, is connected 
with the magnitude S of the bordering layer of it. In general we 


0c 077 . i 
shall have a relation: so Tas , from which follows, that x can 
Ox ° 


only be a linear function of 7’ in the case, when c is mdependent 
of |S. From our measurements however we must doubtlessly con- 


2 


ou 


that therefore ¢ must really be dependent upon S. This fact proves 


clude, that generally can not be supposed equal to zero, and. 


at the same time, that the specijic heat of the surface-layer must 
have another value than for the remaining part of the liquid. The 
surface-energy therefore cannot be completely of a potential nature, 
but partially it must be considered as being of kinetic origin. In 
what manner however it will vary with the state of proceeding 
polymerisation or depolymerisation of the liquid, we cannot tell in 
advance; and the same is the case mtatis mutandis with the depend- 
ence of g upon ¢. 

At the same time it is not superfluous in this connection to fix 
the attention upon the fact, that it cannot be permitted to make 
any definitive. statement") concerning a high degree of association 

uw 

in the case of molten salts, because the observed values of a are 
very small, and the w-teurves seem to approach in these cases much 
better to the rectilinear type 2. For the whole theoretical exposition 
of Eérvés cannot be applied to cases like the present one, where 
nobody can know a priori, if the law of corresponding states will 
be valid. It is just the question, if the measurements still to be 
made will permit us to draw general conclusions upon an analogous 
connection between the temperature-coefficients of the molecular 
surface-energy and the degree of association of such electrolytes? 
Such conclusions could only be esteemed sufficiently justified, if 
certain analogies in the behaviour of molten salts and of the organic 
liquids should be found; at this moment we are still far distant from 
the time, when we shall be able to give any definitive judgment 
upon this matter. 


1) Vide e.g. the relating views of Watpen, Bull. of the Academy of Petrograde 
loco cit. 


421 


§ 4. The rather appreciable differences of our results with respect 
to the variations of w and xy with the temperature, with those of 
other investigators, who bave principally worked after the method 
of capillary ascensions, have suggested to us to investigate in detail, if 
perhaps in our way of working certain factors could be present, 
which may cause systematical errors in any direction ? 

First it was noted, that besides the particular shape of the mentioned 
curves, also the absolute values of y, determined by us and already 
by Feusten, were generally somewhat higher, than those obtained 
with the same liquids by other experimenters and by other methods. 
Of course it is very well possible, that e.g. the lower values published 
by Ramsay and Suieips, and obtained by them by means of the 
method of capillary ascension, are caused by the fact, that the 
moistening of the glass-walls in their capillary tubes has been not 
so complete, as is supposed in the theory of the phenomenon. In that 
case the angle of contact gy will play again a role; and because the 
height of ascension ceteris paribus is proportional to the cosinus of 
the supplementary angle of y, there could thus really be found a 
cause, which would make their results appear smaller, than those 
obtained in our work. 

But moreover we were able to prove on the other side, that our 
values for z, calculated after Cantor’s theory, must surely appear 
somewhat higher, than they really are, because in praxi_ the 
conditions are not completely fulfilled, on which is based the 
deduction of the jinal formula between H, d; and 7 in Canror’s 
theory. 

Let us start with the somewhat more summary deduction of his 
formula by Frusre.’). From this deduction as it is found in the 
paper of this author, it can be seen, that the formula of Canror 
ean have only validity in the special case that the angle 6, which 
the tangent in every point of the sharp edge of the capillary tube 
drawn in any azimuth to the rotation-surface of the small gasbubble, 
makes with the horizontal surface of the liquid, — differs only slightly 
from 90°; in that case 6 = 90° —s, wherein « bas a very small 
value. Some years ago prof. Lorentz was so kind as to draw my 
attention to the fact, that this limiting supposition can be avoided, if 
one makes a few simple substitutions in the two formulae of FrusrTut ; 

2x 1 


—cosA0=r.d, 


ti ; i COs Oy 


and 


1) R. Feusret, Ann. d. Phys. loe. cit. 


oc 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


ote d; . sin 6 y. di 2 
H = —_____—_ + ——_— | ¢9s 9 + ———_—_}, 
cos G (1 — cos 6)? 3 sin @ 1 — cos A 


2) él 
by putting: ¢g = — 3 and) —— Fe Where » is the radius of the 
rT . ht r.cdt 


capillary tube, and y and // are the known symbols. 
The mentioned formulae can by this substitution be changed into: 


1 1 1 


(= en p=gsn@ + ct 48 ie 
4 cos 6 sin* (9/,) ; : 3 © sin O sin® (’/3) 


Table of Corresponding Values of 


0, q and p 

0 q p 
0° ea) (co) 
10 4399.4 793,94 
20 292,60 100,080 
30 61,717 30,86 
40 23,850 15,33 
45 16,458 15,21 
50 12,192 12,06 
55 9 588 9,995 
60 8,000 8,660 
65 7,098 7,862 
70 6,753 7,546 
710 31/43” 6,750 7,542 
715 7,033 7,814 
80 8,433 9,183 
85 13,770 14,479 
86 16,567 17,269 
87 21,277 21,960 
88 30,764 31,448 
89 59,35 60.027 
89°4 63,44 64,12 
90 oe) co 


Now it is possible to calculate for a complete series of values of 
6, the numbers p and g, and to plot them against each other with 
respect to rectangular coordinate-axes. If /7 is measured, and 7 and 
d, are known, p can be caleulated for every experiment, and from 
the diagram the corresponding value of qg (and therefore also of x) can 
be immediately found. The following table gives a survey of the 
corresponding values of p and q, for a series of angles 6 between 
OprandeoO 2s. 

From this table it is seen, that » and qg reach simultaneously a 
mininiun tor 6= 70° 31'43", and that Canror’s formula is properly 
only valid without appreciable error for values of ¢ between O° and 


423 


0°55'. The corresponding curve generally deviates only a little from 
a straight line; however we found that this deviation is yet sufficient, 
to make a correction necessary for all numbers, caleulated from 
Cantor’s formula. 


§ 5. From a special case we can now see easily, that the cal- 
culation of the results in this way and from Cantor’s formula, w7// 
never cause an appreciable change in the general shape of the p-t- 

. . Ou 

curves, and therefore neither in the deduced values of =f the deviat- 
at 
ion of a linear relation between p and q is between 6= 70 31'43" 
and 90° only so slight, that a somewhat important deformation of 
the mentioned curves cannot be the result of this difference in com- 
putation. However there will be caused a parallellous shift of every 
curve, which will dininish the absolute values of % and w with a 
small amount. That this influence is not at all without importance 
in the cases hitherto investigated, may be proved in the following 
way. We choose for this purpose two extreme cases of the here 
studied liquids: diethylether, because the observed values of H are 
here the smallest, and e.g. a substance as resorcine-monomethylether, 
whose values for // belong to the rather great ones. The caleulation 
is made as follows: HZ in m.m. of mercury (O| C.) is multiplied by 
the specific weight of mercury, and this number divided by the 
product r.d,, (r being expressed in mm.). With the obtained value 
for p, the corresponding value of g is found from the table or the 
diagram; this divided by 2 and multiplied by the product 7? .d,, 
gives y% in mG. pro m.m; the number is reduced to Erg pro cm?, 
by multiplication with 9,806, 


Diethylether. 
yinErg. yinErg. winErg. win Erg. 

Us p J em. em.-?(Cantor) em.-2  em.-? (Cantor) 
MOL MOOLOD Ao, 28,9 574,7 582.8 
=20°.5 30,60 29,89 21,5 PLS) 456,2 464,7 
OF Deets) Da ats! AIG 19,6 415,8 424,5 
1 SSR WOW ally) 18,4 392,0 402,9 
EP DESI DSO0) AUT viel 3 74,2 380,0 
292.6 25.30 2470 A6y4 16,8 365,9 374,8 


The whole y-tcurve is thus parallellously shifted to an amount 
of — 0,4 Erg. 
28* 


424 


Resorcine- Monomethylether. 


yin Ere. yin Erg. win Erg. win Ere. 

be P gq ems? em.?(Cantor) em.? cem.-?(Cantor) 
== 20° 62785 62520) -83; 83,9 1850,1 1867,9 
OS Sees) SOB) = bul 52,4 1161,9 ORS 
46° 34,91 34,30 43,4 44,2 1001,6 1020,1 
NMOS aileils sil no) eC) 38,3 896,7 915,8 
166° 2848 27,80 31,5 32,3 782,0 801,8 
206° 25,29 24,60 26,8 27,6 682,6 703,0 


Here is the y-d-ecurve shifted totally to an amount of —0O,8 Erg. 


This is the correction to be applied, and which was already 
indicated in our first communication’); it has been taken into account 
since in every case in all the tables. It may here be repeated once more, 
that although the absolute values of the surface-energy really have 
approached closer by it to the values formerly published, however 
the shape of the y-¢, or u-f-curves is not altered by it with respect 
to any particular feature. 


§ 6. Another question to be answered with respect to the obtained 
experimental results, is this, if it may be considered as possible to 
determine the right values of 4, without being embarrassed there- 
with by the influence of the viscosity of the studied liquid? For 
just because the internal friction of liquids always increases rapidly 
at lower temperatures, and an extreme viscosity of the liquid, — even 
if the bubbling of the gas is executed with extreme slowness, — 
will cause, as we have seen, the maximum pressure /7 to appear 
too great from all kinds of disturbing effects, — the influence 
of this viscosity could perhaps be advanced as a cause of such a 
deformation of the y--curves, that they just would manifest a steeper 
temperature-gradient at the lower temperatures than at the higher. 
Therewith an explanation of the curves of type 3 would be given; 
but it must be here remarked already in advance, that such a cause 
could hardly be adopted for the presence of the curves of type 1, 
just because all viscosity-curves have themselves the shape of type 3. 
However there seem to be many reasons, not to attribute too higha 
value to this explanation of the curvature of the «-¢-lines, even not 
in the case of type 3. 


In the first place it must be remarked, that the curvature of the 


1) I’. M, Jarcer, these Proc., Comm. I, (1914). 


425 


said curves does not run parallel to the variations of the viscosity 
with temperature. Most strikingly this can be seen in those substances 
where the curvature is so slight, that the curves can be considered 
to be straight lines: with ethylbenzoate, whose viscosity at 10° is 
about six times that of acetone, and in a temperature-interval of 
50° decreases to two or three times that value, the y--curve is a straight 
line; with the tsobutylbromide, whose y-t-curve between O° and 85° 
ean be considered as a straight line, the viscosity decreases to less 
than half its original value (from 0,008 C.G.S. to 0,008 C.G.S.) ; 
etc. Neither does the curvature of the y-¢-lines seem to be inmediately 
connected with the absolute value of the viscosity : with acete acid, 
whose viscosity is about three times, with salicylic aldehyde, whose 
viscosity is four times, with pyridine, whose viscosity is about twice, 
with pheneto/, where it is circa three times as large as that of 
ethylalecohol, — in all these cases the curvature of the z-écurves is 
less than for the last mentioned liquid, because they are almost 
straight lines; and with the amine and nitrobenzene, whose viscosity 
is about eight or ten times as great, as that e.g. of the edhylformiate, 
the z-t-curves are even slightly convex. In many cases the y-¢-curves 
will show a more rapid and steeper curvature at the higher tempe- 
ratures, where the viscosity becomes smaller; and the part of the y-¢ 
curve between — 79° and O° is often almost a straight line. With 
.the ethylalcohol the viscosity is about three times as great as in the 
ease of ethylacetate or eihylformiate, but notwithstanding that, the 
y-t-curves show in all three cases about the same curvature. 

To be sure, we have met during our measurements numerous 
cases, where very clearly the impossibility was shown, to determine 
the surface-energy dependently of the viscosity. But this we 
observed only, where the viscosity reached such enormous magnitude, 
that the liquid became glassy or gelatineous, and did not or hardly 
move on reversing the vessel. Such cases we found in: methy/- 
cyanoacetate, methyl-methylacetyloacetate, diethylbromomalonate, cie- 
thylbenzylethylmalonate ; in undercooled dimethyl-, and diethyltartrate 
and a-campholenic acid, and very strikingly with salo/ and resorcine- 
monomethyl-, or dimethylethers. 

Even in these unfavourable cases we succeeded sometimes in 
making some good measurements ; but in most cases this appears to 
be impossible, which is shown by the fact, that even with so small 
a velocity of formation of the gas-bubbles as 50 to more than 209 
seconds, it proved to be impossible to find a maximum pressure 
fl, which really is independent of the speed of the nitrogen- 
flow. 


426 


The behaviour of such extremely viscous liquids with respect to 
the gas-bubbles produced in them, is very variable and often very 
peculiar: in this ease the bubbles are hardly loosened from the 
capillary tube, in that case one observes a periodic increase and 
decrease of the gas-pressure, without a bursting of the bubbles 
occurring ; in another case a very large bubble is produced, which 
suddenly explodes into a great number of very small bubbles ; but 
in no case a maximum pressure can be measured, which is really 
independent of the speed of the gas-flow, proving that it corresponds 
to a real state of equilibrium of the gas-bubble. And this last men- 
tioned fact is so characteristic for all our other measurements : 
within rather wide limits one can vary the speed of nitrogen-jlow, when 
working with ordinary liquids, without a measurable change in the 
determined pressure H_ being observed. On the contrary we studied 
a long series of very thin liquids: e.g. ethylalcohol, diethylether, ethyl- 
formiate, ethylchloroformiate, acetone, methylpropylcetone, chloroform, 
ete., cooled to —-80°C., which notwithstanding the low temperatures 
gave very reliable values of //7; the occasional fact that the temperature 
is so low, can therefore neither be considered of high importanee 
for the abnormally high values of y and w observed. However it 
must be said in this connection, that E6rvés’ relation can no longer 
be considered as valid at temperatures, lower than about half the 
absolute critical temperature of the studied liquids. 

In this connection it is not superfluous to remark, that with liquids 
whose volatility is very great, and which therefore possess at higher 
temperatures a very considerable vapour-tension, there is often some 
difficulty in obtaining reliable values for 7, this maximum-pressure 
being apparently somewhat increased. However the right value can 
be deduced in such cases by often repeating the adjustment of the 
capillary tube, until a really reproducible value will be found. The 
influence of these abnormally high vapour-tensions cannot be of 
essential significance, if the measurements are controlled accurately 
and often carefully repeated. 

All arguments taken together, we think it really very improbable, 
that the changes in viscosity of the studied liquids could be argued 
as the chief cause of the observed curvature of the y-¢- or u-t-curves. 
But in cases of abnormally great values of the viscosity, the deter- 
mination seems doubtlessly no longer possible after this method in 
any exact way; however with liquids, whose viscosity comes e.g. 
very near to that of glycerine, or is even somewhat greater, such 
measurements are already quite reliable if only the formation 
of the gasbubbles takes place ewtremely slowly: in this way for 


427 


instance we found again reliable values with: déethylimalonate (—20 
and butyl-, or tsobutyl-cyanoacetates (—22°). 

Therefore we think it right to draw the conclusion, that the non- 
linear dependence of 7 on the temperature, must be connected with 
the very nature of the surface-energy itself, and that it will manifest 
itself always, as soon the studied temperature-interval is only wide 
enough. 

We can also mention here the fact, that in the ease of 
molten salts, even at very high temperatures and with very small 
viscosities of these liquids, we observed just the same three types of 
y-t-curves: so with potassiwmiodide the type 3, with potassium- 
metaphosphate the type 1, with many others the rectilinear type 2, 
— without it being possible to indicate an immediate reason for it. 
Finally we can draw the attention to the fact, that notwithstanding 
the fact that these determinations range over a much smaller tem- 
perature-interval, some y-écurves of other experimenters (vide e.g. 
Guye and his collaborators) show, on better consideration, also clearly 
a deviation from the rectilinear type; for water this has moreover 
already been mentioned before. 


§ 7. Finally it is bere the place to discuss some points connected 
with the relations between the magnitude of w and the chemical 
constituents of the studied liquids, in so far as we may draw con- 
clusions about it already with respect to the sparing experimental 
data. Moreover the investigations relating to this subject will be 
continued in this laboratory in a quite systemaucal way, because a 
great number of problems have risen in this respect, which only by 
collecting a more extended experimental material can be answered 
by generally acceptable views. The facts hitherto gathered are 
principally adapted, to bring the values of u in qualitative connect- 
ion with the homology of some analogous compounds, and with the 
substitution-relations between some organic derivatives. This can be 
executed best by comparison of the a-¢-diagrams, which were published 
in the successive communications. 


A. Homology. 
Of homologous series we can mention the following: 
Ethylalcohol. Bthylformiate. Ethylacetate. 


1.) n.-Propylalcohol. *) Ethylacetate - *) Amylacet ate. 
Isobutylalcoho!. 


428 


Methylisobutyrate. Acetone. 6 Bthylacetyloacetate. 
4.) Ethylisobutyrate. ’) Methylpropylcetone. *) Eiirylpropyloacetate. 
Tsobutylisobulyrate. 
Tsobuty!cyanoacetate. \ Diethyloxalate. Dimethyltartrate. 
Amylcyanoacetate. ae | Diethylmatonate. , | Diethyliartrate. 
Dutyleyanoacetate. 
*\ Propylcyanoacetate. 
| Ethylcyanoacetate. 
| Methyleyanoacetate. 
10 | Trichloromethane. | Benzene. o \ Nitrobenzene. Aniline. 
"| Tetrachloromethane. Toluene. ~) 0-Nitrotoluene. ~” ) o-Toluidine. 
ll. p-Xylene. 
Mesitylene. 
| Pseudocumene. 
Anisol Resorcinemonomethylether. Methylbenzo ate. 
: | Phenetol. é | Resorcinedimethylether. 16. { Hthylbenzoate. 


Benzylbenzoate. 


Methylsalicylate. Pyridine. 
17.) Ethylsalicylate. ‘) a-Picoline 
Phenylsalicylate. 


By such a comparison of the results obtained we can now derive 
the evidently general fact, that the values of the molecular surface 
energy at the same temperature increase in homologous series, if we come 
to terms of higher hydrocarbon-radicals. Although quantitative relations 
do not so. strikingly come to the foreground, it seems however to 
be clear, that the influence of the same increase in this respect, 
becomes smaller within the series, if the molecular weight of the 
compound increases; a fact, that must be thought also completely 
comprehensible. In most cases these rules hold, as the following 
instances may prove: The value of w is at the same temperature 
greater for isobutyl-alcohol, than for normal propylalcohol, and here 
again greater than with ethylalcohol; just so with ethylacetate greater 
than with ethylformiate, with amylacetate greater than with the 
corresponding ehylether; it is greater for isobuthyl-isobutyrate than 
for the ethylether, and here again greater than for methylisobutyrate ; 
with ethyl-propylacetyloacetate greater than for ethyl-acetyloacetate. 
In the series of the six cyanoacetates, the value of «is greatest with 
the amyl-ether, and decreases here regularly within the series till 
the methylether is reached, while the temperature-coefticients remain 
almost the same; the zsohuty/-ether however has another value for 


Ou 
- and values for uw, which are only partially greater than for the 


429 


propyl-ether: in this also a manifestation must be seen of the differ- 
ences between normal and ramified carbon-chains. In the same way 
the molecular surface-energy of diethyltartrate appears to be greater 
than of dimethyltartrate. In the series of aromatic hydrocarbons, the 
curves for pseudocumene and the isomeric mesitylene are situated 
highest; then follow successively: p-xylene, toluene, and benzene; in 
the same mw is greater for o-toluidine than for aniline, for o-nitrotoluene 
greater than for nitrobenzene; just so for phenetol greater than for 
anisol, for dimethylaniline greater than for aniline, and for a-picoline 
greater than for pyridine. The only exception to this rule hitherto 
found, is presented by the resorcine-monomethylether, which possesses a 
ereater molecular surface-energy than the corresponding dimethylether. 

The substitution by means of members of the aromatic series has an 
analogousinjluence as by those of the aliphatic series, but it is much more 
intensive: in the series of the benzoates, the value of u for the ethy/-ether is 
indeed, greater than for the methyl-derivative, but for the corresponding 
benzyl-ether it is excessively much greater; in the same way it is 
the case with methyl-, and ethylsalicylates and salol, and with methyl- 
propylcetone on one side, and acetophenone on the other. 

B. Relations of Substitution-derivatives. 

The conclusions, which in this respect can be drawn hitherto, 
can be summed up shortly in the following rules: 

1. The substitution of H by halogens is accompanied by an inten- 
sive increase of the molecular surface-energy at the same temperatures; 
the injluence increases evidently with augmenting atomic weight of the 
halogen. 

So u for chlorotoluene is greater than for slorotolwene*), and here 
much greater than for todwene itself; for bromobenzene ai is greater 
than for chlorubenzene, and appreciably greater than for benzene; 
with the m-dich/lorobenzene it is greater than for /lworobromobenzene, 
showing that the specific influence of fluorine seems to be less than 
the difference between bromine and chlorine. In the same way the 
ralue for diethylbromomalonate is appreciably greater than for dietyl- 
malonate; for tetrachloromethane just so greater than for chloroform. 

2. Vhe substitution of N-atoms for C-atoms, or of that of negative 
nitrogen containing radreals for a H-atom, is followed by a relatively 
great increase of the molecular surface-energy at the same temperatures. 


+) The relatively small differences caused by the structural isomerism of these 
compounds, is here neglected for the present; generally the pava-substitution seems 
to be of the highest, the meta-substitution of the smallest influence in this respect. 
We will discuss this peculavity afterwards by considering the results of a special 
set of measurements. 


430 


So yt is appreciably greater for o-nétroanisol, than for anisol; for 
o-nitrotoluene much greater than for ¢olwene; for nitrobenzene much 
greater than for benzene; for aniline and o-toluidine, much greater 
than for benzene ov toluene. Just so for pyridine appreciably greater 
than for benzene; ete. 

3. The substitution of aromatic hydrocarbon-radicals instead of 
H-atoms makes the values of the molecular surface-energy also con- 
siderably greater. 

So the values for sa/o/ ave much greater than for the other 
salicylates; of benzylbenzoate it is much greater than of both the 
other benzoates; of acetophenone much greater than of démethylcetone 
or methylpropylcetone; of diethyl-benzyethylmalonate much greater than 
of diethylmalonate itself; ete. 

Only continued investigations in this direction can however, as 
has already been said, prove with more certainty, if these rules may 
be considered as general ones. Researches of this kind will be 
started in this laboratory within a short time. 


Laboratory for Inorganic Chemistry 
of the University. 
Groningen, June 1914. 


Mineralogy. —* On the real Symmetry of Cordierite and Apophyllte”. 
By Prof. H. Haca and Prof. F. M. Janerr. 


§ 1. In continuation of our investigations!) on the symmetry of 
erystals, which can be discerned as mimetic or pseudosymmetrical, 
we will give in the following a review of the results obtained in 
our experiments relating to the cordierite (tolite; dichroite) and to the 
apophyllite (albine; ichthyophtalm). Of both kinds of silicates specimens 
of dijferent localities were at our disposal, — a fact, which hardly 
can be over-estimated in the study of ROnreEN-patterns, as will be 
proved below. We will describe in the following pages successively 
our observations with: a) Cordierite; b) Apophyllite. 


§ 2. «a. Investigations on the true symmetry of Cordierite. 

Cordierite, asilicate of the chemical composition: H,( Mg, Fe), Al,Sz, ,0,,. 
belongs to those minerals, which lke the arragonite, imitate the 
habitus of hexagonal crystals by means of particular polysynthetical 
twinformations. In literature it is only mentioned, that it is “rhombic” 


1) Haga and F. M. Jagcer, these Proceedings, XVI. p. 792. (1914). 


431 


(a: b:¢ =0,5871 :1:0,5585), but it is evidently unknown, to which 
symimetry-class of the three possible ones it belongs. Its pseudohexagonal 
habitus is obtained in two ways: a. by twin formation parallel 
to {110}, consisting in an intergrowing of ¢hree individuals in such a 
manner, that the faces of {110} will function as the apparent prism- 
faces of the pseudohexagonal combination; 4. by a twinning parallel 
to {130}, in which three_ individuals form either a threefold twin 
by contact, or a threefold one by imtergrowth, the faces of {110} 
being turned outward (fig. 1a). In crystals of the structure, described 
sub a, a plate cut perpendicularly to jOOL{, will appear to be divided 
into six sectors, of which every one is optically biaxial, the planes 
of the optical axes being situated in three successive sectors under 60° 
one to the other, while they are of course equally directed in every two 
diametrically opposite sectors. In crystals of the type 4 there will 
be either three sectors, in which the axial planes are orientated 
along the larger diagonal of the kite-shaped sectors (fig. 16,); or 
there appear six sectors, in which the axial planes are orientated 
perpendicularly to a diameter of the rhomboidal boundary of the whole 
complex (fig. 16,); in this last mentioned case the axial planes in 
two diametrically situated sectors will appear, as in the case sub a, 
orientated in the same direction. The considered possibilities are 
elucidated by some schematical drawings in fig. 1. 


(ii {ft) 10)’ 010) (iio) (iio) cs 
=f ane s™~ 5 oo) 9 
(730) coe (130) f Sp (Seca | 2 | 
“ ev « | < y " 
(070) (20:) (e10) (o10)| e--0 >< e-e-@ | (0 (110)} % P \(ilo ’ | be EY 
4 22 | Sal y e cc3o | 
(130) y /(190) (10 Atel SS eae , L POC ‘iio (0) ane (110)' 
(110) ——— “( 110) Sales SIL ~Y 
(100) 7 
Single Cristal re £ b, 
Vig. 1. 


In most cases the boundaries of the sectors are not distinet; the 
different individuals on the contrary, will penetrate each other 
partially. The cleavage occurs parallel to {O10}, but it is not very 
distinctly pronounced. The optical axial plane is parallel to {LOO}; 
the c-axis is first biseetrix, and the dispersion is only weak: o<v. 
Cordierite is one of the most striking instances of polyehroitic minerals 
(dichroite); the here used crystals also showed this phenomenon in 


a very marked degree. 


§ 3. In our experiments we could use cordierites of the following 
three places: a colourless cordierite of Madagascar; a pale blue 


cordierite of Bodenmais; and a pink cordierite of Jount Ibity on 
Madagascar. 
a. From a magnificent, almost colourless, homogeneous and single 


crystal of cordierite, after its label from J/adagascar, three plane- 
a parallel plates about 1 or 1,2 mm. thick, 


i) . . 5 5 
'Snkensive Were carefully cut, and the following optical 
| Viele properties of them determined (fig. 2); the 


aa eT | arrows indicate the direction of the luminous 
dight Lac 


(001) | 
| 
| 
| 
| 


vibrations, for whieh the mentioned colours 
were observed in the crystals; obviously 
thus the absorption-scheme with respect to 
the crystal-axes is: a@ >>b>>c. The axial - 
plane was parallel to {100}; the c-axis was 


| del low White 


4 (100) first biseetrix (a). The birefringence is about 
_ | 62 =. 05008, and of negative characters @treqes 
Dery Sight Lilac | IntensVutey of these plates we obtained a R6ONTGEN-pat- 

Fig. 2. tern, after they had been carefully orientated 
in the way formerly described by us.'). The distance of the photographic 
plate and the erystal was 45 mm., while the time of exposure varied 
between 1*/, and 2°/, hours respectively. In connection with the question 
of the orientation, attention must be drawn here once more to the fact, 
that deviations of the theoretically right orientation, even so slight 


that they cannot be controlled any more by means of optical test, 
will however always manifest themselves by a slight dissymmetry in 
the R6OnrGEN-pattern. For instance, the image obtained by radiation 
through {O01} in several experiments, appeared to be always un- 
syminetrical to a more or less degree, while by the optical test in 
any of these cases no appreciable deviation of the optical image 
and of the right orientation of the first bisectrix could be proved. 
Thus even the greatest attainable degree of precision in this orien- 
tation can never exclude the necessity, to acknowledge certain 
imperfectibilities of the expected symmetry of the obtained 
RONTGEN-patterns as of only secondary importance in the com- 
parison of these images. and to neglect them presently in drawing 
conclusions from the photographs. This point must always be con- 
sidered in all following discussions of the obtained results; without 
this restriction it simply appears absolutely impossible to draw any 
valuable conclusion from the results obtained by experiment. At the 
same occasion we wish further to remark, that the use of a phos- 
phorescent screen (species “Eresco”) behind the photographic plate 


1) H. Haga and F. M. Jagaer, these Proc., loc. cit. (1914). 


TABLE I: Cordierite. 


433 


evidently often causes disturbances in two possible ways: (st. by 
increasing appreciably the dimensions of the central spot, because 
of the diffuse light-emission of the sereen; which fact may render 
some of the spots situated in the immediate vicinity’ of the central 
part invisible in the reproductions; and 2". because the impossi- 
bility of pressing the phosphorescent screen over its whole surface 
quite equally against the photographic plate, eventually will cause 
some differences in the intensities of the black spots, which apparently 
create an accidental dissymmetry in the obtained photograph. Also 
both these disturbing effects must be taken into account together with 
the above given arguments, to explain the inevitable imperfection of 
the ROnrGEN-radiograms, thus prepared. 

The R6énreen-patterns, which now are reproduced ‘in fig. 3, 4, and 
9 of plate I, can teach us the following facts: A somewhat more 
accurate study of these photographs will immediately show, that 
the images obtained by radiation through the erystalplates {100} and 
{010}, possess only a dilaterc] symmetry: the molecular arrangement 
of the crystal, seen in the two directions perpendicular to these 
faces, can thus possess only one single plane of symmetry, in the 
first case perpendicular to {100}, in the last one perpendicular to {O10} 
and passing through the c-axis; by both images however it is proved 
indubitably, that axes of binary symmetry are completely absent. The 
image, obtained by radiation through the erystal in a direction perpen- 
dicular to {001} however, must be considered doubtlessly to be symme- 
trical with respect toa set of two symmetry-planes, perpendicular to each 
other ; of course the intersection of these two planes, being the c-axis, 
needs to be an aais of binary symmetry too. On Table / we have repro- 
duced a RonTGenogram of this ease, which shows some dissy mmetries 
by a very small error in the normal orientation; the distribution 
of spots of equal intensity however, etc., suggests the symme- 
trical nature of this radiogram with respect to the mentioned planes 
without any doubt. Of this same crystalplate we obtained some 
more radiograms, which were however not sufficiently intense for 
reproduction; they were somewhat more symmetrical than the pho- 
tograph reproduced here, which fact apparently was caused by a 
somewhat better adjustment of the crystalplate with respect to the 
Ronreen-tube. But an optical investigation of the crystal-plates in quite 
the same position as in which they were during the experiment, allowed 
no distinction of the orientation in the several cases: it must there- 
fore be considered a fact of mere chance, if one gets accidentally 
the right position of the plate, necessary to obtain a pattern, whose 
symmetry approaches the pure one with more or less perfection ; 


434 


and furthermore, as we already mentioned, the accidental situation 
of the phosphorescent screen will play in this question also a more 


or less important role. 


§ 4. The obtained results were so surprising, that we thought it 
necessary to repeat the experiments of radiation through the plates 
parallel to {100} and {O10}, also with cordierites of other localities. 

6. From a beautiful, pink eordierite of J/ount Lhity, Madagascar, 
which had no geometrically definite boundaries, two planeparallel 
plates were cut after {100} and {010} and about 1 m.m. thick. The 
plate parallel to {O10} was distinetly dichroitic : for vibrations in 
the directions of the axial plane it was lilaec-white, for those perpen- 
dicular to it intensively pink. On {100} the colour for vibrations: 
perpendicular to the c-axis was pink; for those parallel to it, the 
plate was almost white. 

In the same way two such plates were cut from a single, short. 
prismatic, chaleopyrite-covered cordierite-crystal of Bodenmais ; it was 
fixed upon an aggregate of chalcopyrite and sphalerite. The mentioned 


fo) 


plates were from 1,0 to 1,1 m.m. thick, and showed no distinet di- 
chroism: the plate parallel to }100} showed hardly any difference of 
colour for two perpendicular directions ; that parallel to {010} was for 
vibrations parallel to the c-axis yellowish-white, for those perpen- 
dicular te it however pink coloured. 

In a quite analogous way as described before, ROnrarNograms of 
these four crystal-plates were obtained. The fig. 6 and 7 give the photo- 
graphs for the erystal from Lodenmais, the figures 8 and 9 those 
for the crystal of Mount lbity *). 

From these ROnTGEN-patterns it can in the first instance immedia- 
tely be seen, that also with these crystalplates all radiograms are 
only symmetrical with respect to one single vertical plane, and 
that in these minerals also binary axes perpendicular to {100} or {010} 
appear to be absent. In connection with the results obtained with 
the other cordierite-plates, it is hardly possible to give any other 
explanation of this, than that the absence of both horizontal binary 


1) The cordierites of /bity are somewhat richer in SiO;, Al,03, and MgO, than 
those of Bodenmais, but their content of iron-oxides is less ; the followimg analysis 
may give some idea of this: 

Ibity : 49.05 9/9 SiO, ; 33.08 /) Al,Og; 11.04 °/) MgO; 5.2%) FeO + Fe,Os ; 
1.649/, HO. 

Bodenmais : 48.58 °/, SiQ,; 31.47%) Al,O3; 10.68°/) MgO; 4.90) FeO; 
1,85/, FeO, ; 0.09 %/) CaO; 1.96%/, H,0. 

Vide also: Wutrine and Oppenueimer, Silz. B Heidelb. Akad. d. Wiss. Abt. A. 
N°. 10. (1914). 


435 


aves and of the horizontal symmetry-plane, is really characteristic of 
the molecular arrangement of the silicate. Founding our statement on 
these experiments, we must therefore draw the conclusion, that 
cordierite is an hemimorphic mineral, belonging to the rhombic-pyra- 
midal class (rhombic-hemimorphie class) of the rhombic system, just 
like calamine and struvite, ete. The threefold twinning-aggregations 
of the cordierite must thus be considered to be real pseudo-hevagonal, 
and no pseudo-trigonal mimetic forms. 

Because all possible space-lattices of the rhombic system, as deduced 
by Bravals, possess vertical and horizontal planes of symmetry, the 
molecular arrangement of cordierite can therefore by no means 
correspond to such a Bravats’ space-lattice. However the pseudo- 
hexagonal symmetry of the mineral, just as its prismatic twinforma- 
tions, seem to indicate with strong emphasis a structure-unit, which 
must be considered derived from the rectangular prism with rhombic 
base, whose angles will differ only slightly (ca. 25’) from 60° or 
120°. The choice between the possible structures is hardly to be 
expected: after SCHOENFLIES’ theory e.g., there will be no less than 
22 arrangements, which correspond to the hemimorphy of the rhombic 
system. (SCHOENFLIES, Krystallsysteme und Krystallstruktur, 1891, 
Sk ZSR)E 


j) 5. A second peculiarity of the obtained R6nrGEN-patterns is this, 
that notwithstanding their agreement with respect to their general 
symmetry, yet appreciable differences in the distribution of the black 
spots show themselves, if analogous crystalplates, but of different 
localities are compared. Even a superficial comparison of the figures 
3, 6, and 8 of plate I to the one side, and of fig. 4, 7, and 9 to 
the other side, is able to manifest the great differences immediately. 
Doubtless all analogous images show a number of common spots ; 
but in every radiogram there are moreover new ones, while even 
homologous spots in the different photographs appear with such 
different relative intensities, that the total aspect of the figure becomes 
a quite different one by it. 

As these photographs were made all under precisely the same 
circumstances, we must conclude from this, that the symmetry of 
a species of minerals being evidently always the same, the number 
and the arrangement of its molecular reticular planes, just as their 
molecular densities, are however variab/e with the special conditions, 
which were prevailing during the formation of the crystals. With 
respect to the erterni/ form of the crystals, this is a fact which has 
long been known, and which can moreover readily be explained 


436 


by the different influences of the factors accompanying the formation 
of the crystals. But from our experiments it follows moreover, that 
the ¢nternal arrangement also, the molecular structure itself, must be 
considered as being variable with those evternal factors; thus to the 
different localities, where minerals are found not only the especial 
differences in habitus of the erystals must correspond, but also some 
variations of its internal structure. With respect to the great signi- 
ficance of this conclusion for the question about the constancy of 
mineral-species in general and about the velations between the 
external forces during the crystallisationprocess and the internal 
crystalline structure, — we must remark, that the correctness of 
our view will be established only — satisfactorily by a great 
number of such experiments, to be made with minerals of very 
different origin and accurately known chemical composition. For 
especially of many silicates, and also of cordierite, it is known, that 
they can be altered under the influence of chemical reagents’); and 
it is very well explicable, if such differences in internal structure, 
as we have stated here, were dependent upon such differences in 
chemical composition, instead of being attributed to the Variation of 
physical factors, whieh may have had a variation of the external 
forms as a consequence, however in the case of cordiriete, these 
variations in chemical composition are only small. Only numerous 
experiments in the direction indicated above, will enable us to decide 
in the alternative. 


§ 6. We have tried to prove the hemimorphy of the cordierite, 
just as it follows doubtless from the described experiments, by 
verifying it again by means of the now usual physical methods. 

In the first instance we tried*) to reach our purpose by the aid 
of the wellknown method of corrosion-figures. The plates of cordierite, 
having been carefully cleaned by benzene, afterwards by alechol 
and ether, were submitted during a short moment to the action of 
a very dilute solution of hydrotlhuoric acid; later we made again 
such experiments by means of gaseous hydrofluoric acid and with 
dilute potassiumhydrate-sclutions. In the last mentioned ease, we 
were unable to get any well-shaped corrosion-figures; in the expe- 
riments with hydrofluoric acid however, we always got, even after 
‘) Vide in this respect the paper of WuLrinG and OPPENHEIMER, just published 
in: Sitz. B. Heidelb. Akad. d. Wiss., Abt. A. N°. 10. (1914), p. 5 and 6; 
l,, OPPENHEIMER, Inaug. Diss. Heidelberg, 1914. 

*) In these experiments Dr. A. Siwek has willingly given us his esteemed assist- 
ance. 


437 


the shortest possible action and by means of very dilute solutions 
of the acid, a great number of corrosion-figures, which appeared to 
be elevations, instead of impressions in by far the most cases. They 
generally (fig. 10a, 6, c) did not have any well definiable shape, 
and were moreover quite irregularly distributed over the surface of the 
erystalplates*), only on {O01{ we succeeded sometimes in getting 
some extended rectangular forms, proving the presence of a binary 
axis and of two perpendicularly intersecting symmetry-planes. The 
corrosion-figures on {100} and {010}, and also on the prism {110} 
of the crystals from /bity and Bodenmais, proved clearly in every 
ease the absence of a horizontal plane of symmetry; they were 
however furthermore so abnormally shaped, that they could hardly 
he used for the control of the above deduced symmetry of the 
crystals. This case proves once more, that the method of corrosion- 
figures used, eventually can give unreliable results, either by the 
production of abnormal etching-figures or by a shape of the corrosion- 
figures, which cannot sufficiently exactly be defined. 

A second trial to determine the physical symmetry in this case, 
was based upon the idea, that because the principal axis c was of 
polar nature, it would be possible, that its ends would manifest 
opposite electrical changes on mechanical deformation or on heating. 
Although we are strongly convinced of the truth that a negative 
result can hardly be considered to be a decisive argument in this 
question, we have nevertheless spent a considerable time in en- 
deavouring to prove the polarity of the c-axis by means of Kunpt’s 
method of dust-figures. Although we were able to obtain on this 
oceasion e.g. the alternative red and yellow powdering of the vertical 
edges of prismatic quartz-crystals in a very satisfactory way, however 
all our numerous tentatives with plates of cordierite, as well with 
the pinacoidal as with the prismatic plates, remained without a 
positive result. In every case, if present, this piezo-, or pyro-electrical 
polarity of the c-axis appears to be only so feeble, that it seems 
‘impossible to prove its existence in the described way with any 
certainty. 

It is a quite remarkable fact, which strongly corroborates the 
value of the new method that even where all crystallographic methods 
to find the smaller physical symmetry-differences of crystals used up 
to this date, are failing, the new method however appears to be quite 
able to elucidate the finer feature of symmetry of such crystals in 
so complete and persuading a way. Therefore an indubitable place 


1) In these photographs, the crossed hairs in the field are parallel to the 
directions of optical extinction of the plates. 
29 


Proceedings Royal Acad, Amsterdam. Vol. XVII. 


438 


needs to be reserved in future to the method of RONtGENograms 
among all other crystallographical methods. At the same time however 
it is proved by the results obtained with minerals of different 
localities, how strictly necessary it properly must be considered, to 
build up the whole systematical mineralogy starting from this new 
point of view, and what surprising results are surely to be expected 
therefrom. 

We will now deseribe here the analogous experiments, made 
with apophyllite. 


§ 7. Investigations relating to the Symmetry of Apophyllite. 

For our investigations of the symmetry of apophyllite, we had 
material at our disposal from the following localities: a. from . 
Paterson (U.S. A.); from Bergen Hill, Erie Railroad N.J.; ¢. from 
(ruanajato, in Mexico; d. trom Berufjord in Iceland. The apophyl- 
lites of American origin we will place opposite to that of Iceland 
as a typical group, because they manifest, as will seen below, some 
peculiarities in their molecular structure, which are not present in 
the /celand-mineral, and are substituted in it by other qualities. 

Apophyllite, a mineral with the chemical composition : 

KH,Ca,Si,O,, +45 H,O 
belongs to the important group of the remarkable zeo/ithic silicates ; 
they all contain water, and as was proved for many of them already, 
their vapourtension at constant temperature appears to be continually 
variable with their momentaneous content of water, — a behaviour 
quite opposite to that of hydrated salts in general. The explanation 
of this pbenomenon is commonly given in this way, — which is 
confirmed completely moreover by the physical properties of these 
silicates, — that the water is not combined with the silicate like 
the water of crystallisation, but that it is present, at least partially, 
either in solid solution or hold in the silicate-skeleton by absorption. 

Apophyllite is a typical representative of an optically anomalous 
or mimetic crystal: Brewster in 1819 already discovered the partition 
of the crystal-sections in numerous fields, and since that time the 
pseudo-tetragonal crystals of this mineral have often been the subject 
of research. For the explanation of this anomalous behaviour, two 
theories have been started: in 1877 by Matriarp, who supposed the 
erysials of apophyllite to be polysynthetic twinnings of perpendicularly 
crossed and penetrating monosymmetric lamellae, — the dimensions 
of the monosymmetric molecular-arrangement differing only slightly 
from those ofa tetragonal structure. The second- view, chiefly defended 
by ©. Kiri, explains the optical abnormalities as caused by internal 


439 


stresses, which in their turn are caused by an isomorphous mixture 
of optically positive and negative material '). The supposition of the 
existence of such positive and negative apophyllite-substances which 
is really confirmed in some cases by direct observation, must serve 
at the same time for the explanation of the very weak birefringence, 
and the so-called lewhocyclite-, and chromocyclite-phenomena. We will 
demonstrate in the following pages, that, — waiving tbe question, how 
far the last mentioned phenomena need to be explained by this 
intergrowth of optically positive and negative substances, -— in every 
case the method of the R6nrepn-radiation decides the alternative 
between the two views indubitably in favour of MALiLarD’s hypothesis. 


§ 8. The American apophyllites used were all transparent, pearl- 
coloured crystals; they have a layer-strueture parallel to {001!, to 
which form also the direction of perfect cleavage is parallel. 

Without exception all these apophyllites are optically biaxial in 
convergent polarised light, with positive character of the birefringence. 
The apparent axial angle is only small, with a dispersion: 0 < v. 
By means of a gypsumplate giving the red colour of 1s* order, one 
sees, that numerous blue-, and orange-tinged, rectangularly bounded, 
very small fields are in juxta-, and superposition to each other, as 
in a mosaic; the crystal makes the impression of consisting of an 
innumerable quantity of perpendicularly very small lamellae, which 
evidently are distributed and superposed in very unequal number 
and in a rather irregular way. 

All these preparations give, if the ROnrarnrays are directed per- 
pendicularly to {O01}, the radiograms, which in Table // are repro- 
duced in the figures 1, 2, 3" and 4. Of all these radiograms it is 
again characteristic, that they possess a single plane of symmetry as 
unique symimetry-element ; it is placed in a vertical situation in all 
reproduced figures, and corresponds, as was found later, to a direction 
perpendicular to the axial plane of the optically biaxial individuals. 
The direction of this plane of symmetry can always rather easily 
be fixed on the original negatives by the particular aggregation of 
spots at the upper side of the image, which has the shape of a 
double pinnacle between the two very distinct circular garlands of 
spots there; and also by the facet, that it cuts symmetrically the 
group of the five very intense black spots, which in fig. 1, 8' and 4 
are visible just beneath the centre: in fig. 2 these spots are invisible 


1) The optical phenomena in basal sections of the optically positive apophyllites 
are (after Kooke) exactly analogous to those which would be produced in the 
originally uniaxial crystals, by stresses, working parallel to the edges (O01); (110). 


29* 


440 


on the reproduetion, by the strong radiation of the phosphorescent 
screen and the enlargement of the central spot caused by it, but 
they were distinct on the original photographs. 

It is therefore doubtless, that these photographs can be considered 
to have brought the proof of the fact, that the pseudotetragonal c-axis 
of the apophyllite-crystals, is not even a binary axis; but that at 
best it can be compared with the vertical axis of a monosymmetric 
molecular arrangement: the original molecular structure of apophyllite 
is not of tetragonal, but of monoclinic symmetry. 

We once more emphasize in this connection the existence of the 
group of five intensive spots, just beneath the centre of the image. 
Indeed this garland of five spots, which correspond to five molecular 
planes, seems to be typical for all apophyllites of American origin ; 
it plays evidently in these silicates a preponderant role. As in 
literature there can be found some data, relating to the fact, that 
a heating to 270° C. would be able to expel a part of the water 
and to make the crystal tetragonal in reality, — we have studied 
ihe effect of such a heating at 270° to 300° C. by means of the 
heating-apparatus formerly described by us. And now it was found, 
that all spots disappear, but that the mentioned five intense spots 
are elongated like the fingers of a hand (tig. 36 on plate II). This 
fact could be explained by the supposition that the original sets of 
parallel molecular planes, by which the five intensive spots were 
produced, are changed during the deshydratation and heating gradually 
into the same number of now divergent molecular planes lying in 
five zones respectively. This would be possible, if the molecular 
planes, which are situated nearer to the crystal-surface, will lose 
their watermolecules sooner and more easily than those situated 
nearer the inner part of the crystal: the expelling of the water 
takes place namely very slowly and gradually, while the planes are 
rotating round their zone-axes continually during this deshydratation. 
It is possible, that an analogous, but far more irregular distortion 
of the positions of the molecular planes will be the cause of a gra- 
dually getting vaguer and finally of a disappearing of all other points 
and spots; if not the other explanation, namely that all these points 
correspond to the action of the zafermolecules alone, can be accepted. 
It will be only possible to give some stronger affirmation of this view, 
if more zeolithic silicate will be investigated in an analogous way. 
The fig. 34 is made, after the heated crystal being cooled down 
to the roomtemperature; it appears to be completely identical however 
with the image obtained at 300° C. within the furnace, and it is 
only reproduced here instead of the other, because the last mentioned 


441 


photograph was too pale. The resulting state of the heated apophy llite 
remains thus absolutely fixed on cooling; after the data given in 
literature, the water expelled at 260° C. will be only resorbed after 
about 3600 hours from an atmosphere of water vapour. Anticipating 
on our experiments with the apophyllite of Jceland, we can remark 
in this connection, that with this mineral, which did not show the 
five mentioned spots, there remained nothing at all on the photo- 
graphic plate, after the crystal was heated, except some feeble action 
on the places of the most intensive spots of the original image; 
they only proved, that the transformation by the heating was not 
yet completely finished. In no case we have therefore succeeded in 
proving, as before was done with the boracite, that the pseudotetra- 
gonal aggregation of monosymmetric material, above a certain tem- 
perature can be changed into the really higher symmetrical form : 
instead of such inversion, a change in the silicate-skeleton is pro- 
duced, which at least during the short interval of the experiment 
can be considered to be zrreversible, and which has nothing or not 
directly to do with the real transformation into a true tetragonal 
form. 


§ 9. In opposition to these American crystals, the used apophyllite 
of Leeland must be discerned as a most beautiful, glassy, and perfectly 
clear crystal, which was determined to be a combination of sharp 
pyramid {111} and basal pinacoid {OO1{. The angles of the pyramid 
and of pyramid and basal pinacoid were variable within rather 
wide limits; they deviated from the angles commonly mentioned in 
literature by an amount of cirea 30' to 1°; yet the reflected images 
were splendid and quite sharp, this phenomenon too leading to the 
supposition, that the tetragonal symmetry could only be a mimetic 
one: 

{O01} : {t11} = 59°24’ to 60°13; in literature : 60°32’. 
144} : {4171} ao : ‘5 : 58°56' 
Shea): fe == 74°38! to. 75°39" 3 BO add 


“rather oscillating’’. 


| 


From this crystal two  planparallel plates were cut, the one 
parallel to {OOL}, the other to {100}. 

The plate parallel to {O01} between crossed nicols appeared 
to be not completely isotropous, but to possess an extremely weak 
birefringence, with the principal optical sections orientated perpen- 
dicularly to the edges (110) : (OO1). 

By means of a gypsum-lamella, giving the red of 1% order, it 
appeared to be divided into four sections, of which the diametrically 


442 


Opposed ones were tinged blue, while the other ones were orange. 
Every sector is optically biarial, with positive character; the axial 
plane is in every sector perpendicularly orientated upon the corre- 
sponding edge (110):(O0O1). The four quadrants were limited in the 
centre of the basal section by straight borders, corresponding with 
the edges of the psendo-tetragonal pyramid; in every sector the 
direction parallel to the corresponding edge (110): (O01) is that of 
smaller optical elasticity. 

The plate, which was cut parallel to {100}, showed on very 
strong enlargement and by the aid of a gypsum-plate with the red 
of Ist order, a very fine lamellar structure: the lamellae are super- 
posed parallel to the faces of the pyramidal, apparently tetragonal 
limiting forms, while also locally smaller or more extended fields 
can be discerned, in which the optical orientation appears to be 
different and in an orientation, evidently perpendicular with respect 
to each other. 

Of these plates the RONrGEN-patterns were obtained in the usual 
way: the fig. 5a, plate II represents the image, if the plate parallel 
to }OOL} is radiated through; it corresponds to the centre of the 
basal sections, where the four sections are tangent to each other; 
fig. 6 was obtained by radiation through one single sector, and 
fig. 56 represents the RON?rGENogram, correspondiug to a radiation 
through the plate, cut parallel to {100}. 

Although fig. 5@ appears to be approaching to a much higher 
degree to real tetragonal symmetry, it is easy to recognize in it the 
perpendicularly crossed partial figures of the photographs fig. 1—4, 
but without the formerly mentioned intensive five spots near the 
centre; and fig. 54 shows a symmetry with respect to two planes 
of symmetry, perpendicular to each other, and a binary axis. In 
fig. 6 it would again be possible to doubt this approach to tetragonal 
symmetry; however it seems to be present, and the figure allows, 
e.g. by direct comparison with fig. 4, to prove that in the radiograms 
of the /celand-apopliyllite doubtlessly several elements of the mono- 
symmetric American structures are present. From all these peculiarities 
it seems that we may conclude, that the image of the apophyllite 
from Iceland approaches only therefore more that of a real tetragonal 
crystal, because the intergrowth of the monoclinic lamellae is in this 
case much finer and more regular than in the American species; 
and with this doubtlessly the other facet is connected, that the 
Iceland-mineral looks so much clearer and within larger sectors 
more homogeneous, than the turbid-looking and opaque American 
apophy llites. 


445 


Finally we can here also fix the attention to the fact, that the 
RontGenograms of the apophyllites of different localities differ yet 
in their finer features, although they possess the same general 
symmetry. 


§ 10. In our opinion these investigations have decided ‘without 
any doubt between the two prevailing theories for the explanation 
of the optical anomalies of apophyllite, i favour of MaLiarn’s 
hypothesis: not the tetragonal molecular structure, disturbed later by 
internal stresses, must be considered as the primary state of the 
mineral; but this state corresponds to an originally monoclinic 
molecular arrangement, which approaches very closely to a tetragonal 
one, and which reaches its pseudo-tetragonal character by the 
crossing and intergrowth of two such monosymmetric structures, 
by means of polysynthetic lamellar twinning, and a mutual penetration 
in directions, which make an angle of 90° with each other. 


POSTSCRIPT. 


Finally we will use this opportunity, to add here again a con- 


@ 
fe) ® 
® 
Q ® 
(o) 
® Q 
e 2 
@ 
Oo 
2 
— + — —— — —— @Q— ——&) — 
® 
(e} 
e 
= ® 
@ 
S e 
e ® 
® 
® @ 
@ 


Boracite at 300°. C. 


444 


struction-figure, relating {0 our paper on the symmetry of boracite ‘); 
this figure will reproduce the changes observed by us with this 
mineral before and after heating, in a ciearer way, than the not 
very satisfactory photographical reproductions given in that paper. 
In constructing this stereographical projection, Dr. L. S. Ornsrpin 
has given us again his kind assistance, for which we thank him here 
also once more. The change of the binary axis into the quaternary 
one, is proved by this figure again in a very striking manner, and 
it is easy to see, which reticular planes of the molecular structure 
have disappeared at higher temperature. 

At the same time we will correct some errors in the former 
paper, where on p. 797 the words “right” and “left” need to be 
interchanged several times, because the photographs are unhappily 
placed in reversed position, so that on comparison of the text and the 
figures, there is a confusion of right side, left side, and of horizontal and 


© 9 
r) 
® ® @ 
Te ) 
e® @ i) 
Ouike a 
oe 
a ® 
e 
® 
2) © 
@—_®- 
® 
1e) @ 
r) 
& ® 
® 
° 
So © 
e ® ® 
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Boracite at room-temperature. 


') H. Haca and I’, M. Jan@er, these Proc. loco cit. 798 (1914). 


445 


vertical directions. The new figure in this paper has been adjusted in 
such a position, that it will correspond to the text of p. 797, if only the 
words vertical and horizontal (line 9 and 10 from beneath) are inter- 
changed on reading. 


Groningen, June 1914. 
Laboratories for Physics and for Inorganic 
Chemistry of the University. 


Physics. — “FRESNEL’s coefficient for light of different colours.” 
(First part). By Prof. P. Zeeman. 


One of the empirical foundations of the electrodynamics of moving 
bodies in the domain of optics is Fiznau’s celebrated experiment on 
the carrying along of the light waves by the motion of water. Let 
w be the velocity of water relative to an observer, then for him 
the velocity of light propagated in the water wauld be 


- 
CG. === sB07 
u 

if the dynamical laws for the addition of velocities were perfectly 
general. 

In this equation a designs the index of refraction of water, c the 
velocity of light in vacuo, and we must take the upper or the lower 
sign, according as the light goes with or against the stream. Fiznau 


demonstrated that not the entire velocity w but only a fraction of 
it comes into action. This particular fraction appeared to be approxi- 


1 
mately equal to 1 — —, Frusnew’s coefficient. Hence we must write 
3 ae 
in place of the above given formula: 
= c 
Cr SS SSC Joh is Joo antes Me ape (al) 
where 
1 
Sieelettee iii gd callie oy 
we 


For water ¢ is equal to seven-sixteenths. 

The extremely important role which the formulae (1) and (2) have 
had in the theory of aberration, in the development of Lorenrz’s 
electronic theory needs not to be exposed here, and it is hardly 
necessary to state that equation (1) is now regarded as a simple 
confirmation of Einsrrin’s theorem concerning the addition of velocities. 

I may be permitted however to point out the smallness of the 


446 


second term of formula (1). The velocity which we are able to 
obtain in a column of water transmitting light is of the order of 
magnitude of 5 metres per second. We have thus to find a difference 

; 3108 : 
of velocity of 5 metres in 13 m., i.e. Of one part in fifty millions. 

This was done by Fizeav ') in one of the most ingenious experi- 
ments of the whole domain of physics. Fiznau divided a beam of 
light issuing from a line of light in the focus of an object-glass 
into two parallel beams. After traversing two parallel tubes these 
beams pass through a second lens, in the focus of which a silvered 
mirror is placed. After reflection the rays are returned to the object 
glass, interchanging their paths. Each ray thus passes through the 
two tubes. A system of interference fringes is formed in the focus 
of the first lens. If water is flowing in opposite directions in the 
two tubes, one of the interfering beams is always travelling with the 
current and the other against it. When the water is put in motion 
a shift of the central white band is observed: by reversing the 
direction of the current the shift is doubled. 

The ingenuity of the arrangement lies in the possibility of securing 
that the two beams traverse identical ways in opposite directions. 
Every change due for example to a variation of density or of tem- 
perature of the moving medium equally influences the two beams 
and is therefore automatically compensated. 

One can be sure that a shift of the system of interference fringes, 
observed when- reversing the direction of the current must be due 
to a change of the velocity of propagation of the light. 

The tubes used by Fizeau had a length of about 1,5 metres and 
an internal diameter of 5,3 m.m., whereas the velocity of the water 
was estimated at 7 metres. With white light the shift of the central 
band of the system of interference fringes observed by reversing the 
direction of flow was found from 19 rather concordant observations 
equal to 0,46 of the distance of two fringes; the value calculated 
with FRESNEL’s coefficient is 0,404. : 

The result is favourable to the theory of Fresnen. The amount 
of the shift is less than would correspond to the full velocity of 


‘ ? ei: 1 
the water and also agrees numerically with a coefficient 1——, if- 
ul 
the uncertainty of the observations is taken into account. 


) H. Fizeau. Sur les hypotheses relatives a |’éther lumineux et sur une expérience 
qui parait démontrer que le mouvement des corps change la vitesse avec laquelle 
la lumiére se propage dans leur intérieur. Ann. de Chim. et de Phys. (3) 57 
385, 1859. 


447 


Fiznau’s experiments, though made by a method which is theore- 
tically as simple as it is perfect, left some doubts as to their accu- 
racy, partly by reason of the remarkable conclusions as to relative 
motion of ether and matter to which they gave rise, and these 
doubts could only be removed by new experiments. 

35 years after Fiznau’s first communication ') to the Académie 
des Sciences, Micuenson and Moriny*) repeated the experiment. 
They intended to remove some difticulties inherent to Fizeau’s method 
of observation and also, if possible, to measure accurately the fraction 
to be applied to the velocity of the water. Micurnson uses the prin- 
ciple of his interferometer and produces tmterference fringes of con- 
siderable width without reducing at the same time the intensity of 
the light. The arrangement is further the same as that used by 
Fizwau but performed with the considerable means, which American 
scientists have at their disposal for important scientific questions. 
The internal diameter of the tubes in the experiment of Michrtson 
and Moriey was 28 m.m. and in a first series the fotw/*) length of 
the tubes was 3 metres, in a second series a little more than 6 metres. 

From three series of experiments with awhile light Micuuson found 
results which if reduced to what they would be if the tube were 
2 5 metres Jong and the velocity 1 metre per second, would be 
as follows: 


“Series 4A = double displacement 
if 0,1858 
2 0,1838 
3 0.1800” 


“The final weighted value of A for all the observations is 4 =0,1840. 
From this by substitution in the formula, we get «= 0,454 with a 
possible error of + 0,02”. 

For light of the wavelength of the D-lines we calculate 1 

1 at 
— —, = 0,437. This agreement between theory and observation is 

u 
extremely satisfactory. 

A new formula for ¢ was given by Lorentz *) in 1895 viz.: 


1) Comptes rendus 53, 349, 1851. 

2) A. A. Micuetson and E. W. Mortey, Influence of motion of the medium on 
the velocity of light. Am. Journ. of Science (3) 31, 377, 1886. 

8) Viz. the sum of the lengths of the ways in the moving medium, traversed 
by each of the interfering beams, or approximately twice the length of one of the 
tubes. 

4) H. A. Lorentz Versuch einer Theorie dev electrischen und optischen Erschei- 
nungen in bewegten Kérpern, p. 101, 1895. See also Theory of Electrons p. 2¥0, 


1 gn 


=1-- —-——4 Wome AEN oe © sale 
j uw uda (3) 


For the wavelength of the sodium lines this becomes: 
0.451. 

We see, therefore, that the value deduced by formula (3) deviates 
more from the result of the observations than the value given by 
the simple formula (2). 

“Sollte es gelingen, was zwar schwierig, aber nicht unméglich scheint, 
experimentell zwischen den Gleichungen (8) und (2) zu entscheiden, 
und sollte sich dabei die erstere bewahren, so hatte man gleichsam die 
Dorrrer’sche Veranderung der Schwingungsdauer fiir eine kiinstlich 
erzeugte Geschwindigkeit beobachtet. Es ist ja nur unter Beriick- 
sichtigung dieser Veranderung, dass wir die Gleichung (3) abgeleitet 
haben’. 7) 

It seemed of some importance to repeat with light of different 
colours Fizeav’s experiment, now that the correspondence between 
theory and observation had become less brilliant, and in view of 
the fundamental importance of the experiment for the optics of 
moving bodies. 

From the point of view of the theory of relativity the formula (3) 
is easily proved, as has been pointed ont by Lave’), neglecting 
terms of the order sh Recently, however, again some doubt as to 

; 
the exactness of Lorentz’s term has been expressed. I may refer 
here to a remark by Max B. Weinsrein*) in a recent publication 
and to a paper by G. Jaumann *). The last mentioned physicist gives 
an expression for the coefficient ¢, which for water does not differ 
much, but in other cases deviates very considerably from FREsNEL’s 
coefficient. 

The interference fringes were produced by the method of Micuerson. 
The method of observation introduced will be described later on. 
The incident ray s /a meets a slightly silvered plate at a. Here it 
divides into a reflected and a transmitted part. The reflected ray 
follows the path abcdea f, the transmitted one the path 
aedcbha f. These rays meeting in the focal plane of 7 have 


1) Lorentz. Versuch u. s. w., 102. 

2) M. Lauvs. Die Mitfiihrung des Lichtes durch bewegte Kérper nach dem Re- 
lativititsprinzip. Ann. d. Phys. 28, 989. 1907. 

5) Max B. Wernsrery. Die Physik der bewegten Materie und die Relativitits- 
theorie. Leipzig. 1913, see note on p. 227 of his publication. 

) G. Jaumann. Elektromagnetische Theorie. Sitzungsber. d. Kaiserl. Ak. der 
Wiss. Wien. mathem. naturw. Kl. 117, 379. 1908, especially p. 459. 


449 


pursued identical, not only equivalent, paths, at least inis is the 
case for that part of the system of interference fringes which in 
white light forms the centre of the central band. 


Fig. 1. 

In order to verify the formula (3) it is necessary that the light 
be monochromatic. Further it seems of immense advantage to have 
a water current which remains constant during a considerable time. 

For observations with violet light this even becomes strictly neces- 
sary, because visual observations are impossible with the violet 
mercury line (4358) used. MicueLson obtained a flow of water by 
filling a tank, connected with the apparatus; by means of large 
valves the current was made to flow in either direction through the 
tubes. “The flow lasted about three minutes, which gave time for 
a number of obseryations with the flow in alternating directions”. 
In view of my experiments the municipal authorities of Amsterdam 
permitted the connection of a pipe of 7.5 em. internal diameter to 
the main water conduit. There was no difficulty now photographing 
the violet system of interference fringes, though the time of expo- 
sition with one direction of flow was between 5 and 7 minutes. 
The pressure of the water proved to be very constant during a 
series of observations; the maximum velocity in the axis of the 
tubes, of 40 m.m. internal diameter and of a total length of 6 
metres, was about 5,5 metres. : 

Before recording some details of my experiments, | may be per- 


450 
mitted to communicate the general result that for water there eaists 
a dispersion of Fresxwi’s coefficient and that formula (3) and there- 
fore the third term of Loruntz ts essentially correct. 

I wish to record here my thanks to Mr. W. pn Groot phil. nat. 
eand. and assistant in the physical laboratory for his assistance 
during my experiments with the final apparatus. 

The difficulties encountered in these experiments were only sur- 
mounted after two reconstructions of the apparatus. Great annoyance 
gave the inconstancy of the interference fringes, when the pressure 
of the water or the direction of flow were changed. Then not only 
the width of the interfereice bands, but the inclination of the fringes 
were undergoing uncontrollable variations. All these defects were 
perfectly eliminated by the use of wide tubes and by arranging the 
end plates in the manner indicated in Fig. 3. 


I am indebted to Mr. J. vAN Dpr Zwaat, instrumentmaker in the 
laboratory for his carefully carrying out my instructions and designs 
in the mechanical construction of the apparatus. 

In fig. 2A a side aspect, and in Fig. 2B a horizontal projection 
of the arrangement on a scale of about ‘/,," is given (see Plate). 

The interferometer is at the right side, at the left the rectangular 
prism is placed. 

The mounting of this prism is only sketched and was in reality 
more stable than might be inferred from the drawing. 


451 


Prism and interferometer were mounted on the piers cemented 
to the large brick pier of the laboratory. The tubes are entirely 
disconnected from the interferometer and mounted on a large iron 
[ girder; this girder is placed upon piers of freestone cemented to 
large plates of freestone fixed to the wooden laboratory floors. In 
this manner the adjustment of the interferometer cannot be disturbed by 
vibrations proceeding from the tubes. At the right of the horizontal 
projection the four large valves may be seen, by turning which the 
current was made to flow in either direction through the tube systems. 

The mountings containing the glass plates by which the tubes 
are closed are not given in the Plate. One of these mountings con- 
taining the plane parallel plates of glass is drawn to scale in Fig. 3 
at one half of the natural size. The four plates of glass are by 
Hiteer, they are circular of 24 m.m. diameter and 10 m.m. thick ; 
in a second series of observations plates 7 m.m. thick have been 
used. The accuracy of parallelism of the plates is excellent; they 
are indeed cut from echelon plates.. The general plan adopted for 
the construction of the plate mountings is this: one can only be 
sure that no change will occur in the position of the plates during 
the course of an experiment, if this position is entirely dejinite. In 
order to attain this the glass plate rests upon the inner, accurately 
grinded, surface of the brass piece d. This piece d fits accurately 
into the conical inner part of a piece 4, itself rigidly screwed to 
the tube a. Parts d and 6 are connected by means of the counter 
nut c. The glassplate is held against d by the nut e. There is no 
objection to the presence at the zmszde between e and d of rings of 
hard india-rubber and of brass. (To be continued). 


Physics. — “A new relation between the critical quantities, and on 
the unity of all substances in their thermic behaviour.” (Con- 
clusion). By Dr. J. J. van Laar. (Communicated by Prof. H. A. 
LorRENTZ). 


(Communicated in the meeting of April 24, 1914). 


By way of supplement we shall add the calculation of three more 
isotherms he/ow the critical temperature, for which (loc. eit.) data 
are known from the unsaturated vapour region. If the p-values above 
T; were somewhat too high on the whole, now we shall find values 
which are much too low, lower even than #,, and therefore impos- 


sible. These deviating values can only be explained, when with low 
temperatures and large volumes association in the vapour is assumed, 


452 


For then, when R7 in the equation of state is made smaller by a 
factor <1, also v—/ will be smaller, hence 6 greater. In this way 
the too small /-values could therefore be raised to the normal amount. 
We shall see in the following paragraph that inside the region of 
coexistence the same phenomenon takes place: the 4-values in the 
vapour much too small (even large negative), the 4-values in the 
liquid phase normal and in harmony with the theory. 

Something particular takes therefore place for the large volumes: 
there is either association in the vapour, or the values of the pressure 
have been measured too small, or the values of the vapour densities 
too large. We shall presently return to this. 


Ff. Isotherm of —130°,38 = 142,71 absolute. Hence m=0,9473, 
3,424 m = 3,244. 


p dy & | n €+5:n2 n— | B 
| | 
12.773 27.394 0.2661 10.873 0.3084 10.518 | 0.355 
| | | | | 
28.878 77.821 0.6016 3.827 0.9430 3.440 } 0.387 
| 
Mean 0.371 | 


Here we should have y = 0,727, 4, = 0,415, &, = #8, K 1,475 = 0,421. 


Hence the value of ”, found is too low. 


g. Isotherm of — 139°,62 = 133,47 abs. Here is m= 0,8860, 
424 77 = 31034: 


p dy € n e+5:72 n— 


11.986 28.122 0.2497 10.591 0.2943 10.308 || 0.283 
14.586 35.573 0.3039 Sono 0.3752 8.085 0.287 


Mean 0.285 


With 7 = 133,47 corresponds y=0,719, 2, — 0411, 2,— Gee 
<< 1,457 = 0,416. The found value of &,, viz. 0,285, is far below 
the theoretical value O,42. 


h. Isotherm of — 149°,.60 = 123,49 abs. For m is found 


m= 0;8197, so 3,424 m= 2.807. 


—— 


| 

0.2323 | 10.206 | 0.2803 | 10.014 0.192 
| 0.3341 8.401 0.195 
| 


o 
tr 
a 
a 
> 
ioe) 
or 
vo} 
-I 


Mean 0.194 _ 


Here y=0,711, 4 =0,406, &,=8, X1,439 = 0,411; 0,19 
again remains considerably below this. 

Combining the found values of &, in a table and comparing them 
with the theoretical values, we get the following survey. 


m | OS ele AS meets oie elt, OFemenl Ot | 0.95 0.89 0.82 


0.49 0.46 0.435 0.43 0.43 


0.42 0.42 0.41 


| 
B, cale. | 
OF55) v0: SIN O45" 043i 0242 | 0.37? 0.28? 0.19? 


B, found 


As was already remarked above, the great deviation, especially 
below 7i.(m<1), mmst not be ascribed to the theory, but to the 
experiment, or to association in the vapour. 

For the found values of &, become, as we shall see, even negative, 
henee impossible, at still lower temperatures — while also yop, is 
continually fornd smaller than @j,,, which of course points to 
something particular in the vapour: either association, or inaccurate 
vapour- or volume determinations, in consequence of a systematic 
error. (Consult also g. of § 18 for a possible explanation.) 


18. The region of coexistence. (Cf. Comm. 131 and These Proce. 
of Nov. 1913 (Comm. 138)). 

For the calculation of & from the given values of the coexisting 
vapour and liquid densities it is to be regretted that the vapour 
pressure observations (see also Comm. 115) have not been made at 
exactly the same temperatures as the density observations. This has 
rendered interpolations necessary, which of course impairs the 
perfect accuracy of the ¢, which will make its influence felt chietly 
on the #-values which are calculated from the vapour densities. 

In this connection we should not omit mentioning that the value 
of /, caleulated from the first observations of the vapour tensions 
(Comm. 115), is much too low, viz. 5,712, whereas the much better 

30 

Proceedings Royal Acad, Amsterdam, Vol. XVII, 


454 


value 7 > 5,933 follows from the values given in Comm. 1204 
(see p. 10)’). 
We had even sufficient reasons (see § 17) to fix the value of 
7’ at 6 (f could be still somewhat larger then). 
Rankine-Bosr’s interpolation formula (see These Proe. of Noy. 1913, 
or Comm. 188), namely 
c d 


b 
log pa + i Ser 


gives by differentiation : 


hence 


T 2,3 A ied ve Oo 61538,18 32293927 ~ 
Pas aca ity eae Wael eV Yop cesta 2 
tp die OT To) a / 


T? 
But this formula, which is caleulated from all the observations 
of p (so also from those below — 140°,80), and corresponds pretty 


well with it, gives the value /;,= 5,628, which is much too low, 


at 7), (150,65), hence still lower than the value fj, = 5,712, given 
at the conelusion of Comm. 115, and ealeulated with / = — 524,3169, 
c= + 11343,28, d= 0. 

In virtue of this I think I have to recommend caution in the 


use of the values of p, at least in the neighbourhood of the eritical 
temperature. 

We shall now give the following survey of the values found for 
the densities 9, and 9, (Comm. 131), and also the corresponding 
values of p (Comm. 115, and These Proe. of Noy. 1913 or Comm. 138). 


— 125°.17 
— 131°.54 
—. 1359.51 
—— 140°. 20 
— 150°.76 
— 161°.23 
— 1759.39 
— 183°.15 


We 


have 


| 


calculated 


. 771289 
.91499 
.97385 
.03456 
.13851 
22414 
.32482 
.37396 | 


from 


~~ 


Jo 


l 


Vi 


0.29534 
0.19432 
0.15994 
0.12552 
0.06785 
0.03723 
0.01457 
0.00801 


and o 


v2 


| 


p=42.457 (for — 125°. 49) 


35.846 ( >» — 129°.83) 
29.264 (» —134°.72) 
22.185 (» — 140°.80) 
13.707 (» —150°.57) 
7.4332 ( » — 161°.23) 


1.3369 ( » — 183°.01) 


given in the following tables by means of 0; = 0,53078. 


the values of d, and d, 


1) Slightly below 7%, at —125°,49, f = 2,577 K2,3026 = 5,933 was namely found, 


455 


@. t= —125°,17, hence T= 147,92, m= 0,9819, 3,424 m = 3,363. 
By means of linear interpolation p = 42,944 has been calculated, 
so «= 0,8947. 


0.292 0.394 (Lig.) 
1.376 0.421 (vapour) 


0.687 1 11.50 
P07 —l|° 2.443 


d, = 1.4563 
dy = 0.5564 


As theoretically @ ranges from 0,42 to 0,29 (see above), both the 
values found can be correct. 

by = — 131° 54, P= 141,55. Hence m =0)9396, 3,424m= 
= 3,217. Linear interpolation, giving p= 38,545, «= 0,6989, would 
be too uncertain here, as —129°,8 differs too much from —131°,5. 
Van per Waats’ formula — log’ =f gives with /= 2,444") 


_ the value «= 0,6964. 


I 


| | | | 
d | n | e+5 ad? | n—£ B 
| l | 
d, = 1.7238 0.580 | 15.55 0.207 | 0.373 (lig) 
d, = 0.3661 Ques 1.367 | 2.354 | 0.377 (vapour) 


As £2 ranges from 0,42 to 0,29, the @-value in the vapour is too 
small. 

c. == —135°,51 = 137,58 abs. Hence m = 0,9132, 3,424 m=3,127. 
A linear interpolation gives p= 28,344, ¢=0,5905; van per Waats’ 
formula with f= 2,420 gives «= 0,5890. 


| j 
| 


=e = 7 TI 
d n e+5d2 | n—B } B 
| | | 
dy =1.8348 | 0.545 | 17.42 | 0.179 | 0.356 (4ig.) 
d, = 0.3013 3.319 1.043 | 2.998 | 0.321 (vapour) 


1) The values of f have in each case been calculated by me from the vapour- 
pressure observations. 


30* 


456 


The .2-value in the vapour begins to be smaller here than that 
in the liquid! 


d. t= —140°,20 = 132,89 abs. Hence m=: 0,8821, 3,424 m=3,020. 
For p we find through linear interpolation p= 22,795, ¢=0,4749; 
from — log’ «= ete. with f=2,415 on the other hand «= 0,4757. 

d n |) et5d2 | n— & 


d; = 1.9491 0.513 || 19:47 ety te 
| | | 


0.358 (Lig.) 


| 0.230 (v.) 
| 


48, should be about 0,42. Besides 0,23 is again < 0,36. 
@) $= —150°176 = 122533 abs.; Hence yn 0138120, 33404 7— 
= 2.780. Linear interpolation gives p = 13,595, « = 0,2832. 


d>—=0.2365 | 4.229 || 0.7553 | 3.999 


1 e+5a2 | n—Z B 
| ) 
|| || 
d, = 2.1450 0.466 || 23.29 | 0.119 | 0.347 (Lig) 
dy=0.1278 | 7.823 | 0.3649 | 7.619 | 0.204 (v.) 


| 


The value of @, is 0,41; 0,20 remains far below this. We moreover 
point out that also / of § 17 at t= — 149°,6 yielded a perfectly 
harmonious value for the vapour, viz. 0,19. The two series of 
observations, therefore, cover each other entirely. 

f. t= 161°,23 = 111,86 abs. From this m = 0,7425, 3,424 m = 
= 2,542. Linear interpolation gives p= 17,4332, «= 0,1549. 


d n We 52) n= G | B 
| || \| 
d; =2.3063 | 0.434 || 26.75 0.095 |, 0.339 (lig.) 
d>— 0.07014 | 14.257 | 0.1795 | 14.167 | 0.090(v.) 
| | | 


£2, begins to be more and more impossible. We point out that 
when f— 1 is iaken not =5, but e.g. =4,95, the value 
Bi,, does not appreciably change: 0,339 then becomes 0,338. But 
2, would then become still smaller, viz. 0,07 instead of 0,092). 


If p=7,58 instead of = 7,43, so ¢ = 0,158 instead of = 0,155, we should 
also have found 0,34 for the value of g in the vapour, the same value at 
least as that for the liquid. (Also the ,assumption °, = 0,C366 instead of 0,0372 
might lead to the desired purpose). 


vA¥ 


457 


g. 1=—175°,39 = 97,70 abs. Hence m = 0,6485, 3,424 m = 2;221. 


The value of « interpolated from —/og™ «= ete. with f= 2,322, 


gives ¢ = 0,05518. 


—— ——— ——- ——— 
d n € +5 @?2 n—P ie) 
d, = 2.4960 0.401 31.21 0.071 || 0.329(diq.) 
dy = 0.02745 | 36.43 0.05894 | 37.67 —1.24!(v.) 


Can the clue to the singular behaviour of the vapour perhaps be 
found in this that Crommenin has not determined the vapour densi- 
ties directly, but that he has calculated them from the law of BoyLE? 
With a too small value of » one naturally gets then a too slight 
value of @ from @ =n — (38,424 im: ¢). Then no association need of 
course be assumed in the vapour, and the impossible values of 2, 


below 7%. are at once accounted for. The found values of 2, would 
then be quite worthless. The question is therefore: where has 
CromMeLIn begun not to determine the given values of the vapour 
| density directly, but to ca/cuéate them from the (not yet valid) law 
of Borin ? *) 
he t= — 183° 15=6994 abs. Here m= 035970, 3.494 m = 2.044. 
From /og'*e= etc. we find the value «= 0,02742 (p = 1,3162) 
with f= 2,314. 


dy | a i etsa| ne | |B 


OS SF SS SSS SS ; 
d; = 2.589 | 0.386 || 33.53 | 0.061|| 0.325 (dig.) 


dp = 0.01509 66.26 |) 0.02856 | 71.87 | --5.31! (2) 
| | 

We point out that the liquid value duly decreases gradually, and 
is still higher than 8, = 0,29 at 7’ = 90 (absolute). So there is nothing 

impossible here °*). 
1) Otherwise p= 2,78 would have to be taken here instead of 2,64, hence 
, e — 0,058 instead of 0,055; or else o; should be assumed somewhat smaller, in 
order to find at least the value 0,33 (that of the liquid) for 8 


vapour’ 
2) A rise of p to 1,44 instead of 1,32 (s to 0,030 instead of 0,0274) — or else a 
diminution of 03 from 0,0O8O ts 0,0075 — might reduce 6, to 0,33 here. The 
first supposition is impossible, for then the value of p at —183°,15 would be 


greater than at 183°,01, where 1,34 was found. But a diminution of g. by 6%/, 
in consequence of an erroneous calculation of e, (probably from the law of Boyte) 
is very well possible. 


458 
Summarizing, we get the following survey for the region of coexistence. 


m | 0.98 0.94 0.91 0.88 0.81 0.74 0.65 0.60 


| 


Blig.| 039 0.37 0.37 0.36 0.35 0.34 0.33 0.325 
Bo. | 0.42 0.38 0.32? 0.23? 0.202 0.09? —1.24? —5.3? 


At the lowest temperature, viz. t= 89,94 abs., y would be about 
0,688, and 8, accordingly 0,393, 8, = 8, « 1,889 = 0,397, so that 
8 ranges from about 0,40 to about 0,29. The liquid value 0,825 at 
n= 0,4 can be in harmony with this. 

In order to examine whether the values of Biiy. also agree quan- 
titatively with our theory, we will in the first place indicate for the 
different values of 7(m) the corresponding values of m and y (caleu- 
lated from 2y — 1 = 0,038 V 7). Besides the value of v: vy, =v: bd, = 
=n: 8, is given. (8, = 0,286). 


m | 0.98 0.94 0.91 0.88 0.81 0.74 0.65 0.60 0 
n | 0.687 0.580 0.545 0.513 0.466 0.434 0.401 0.386 | 0.286 
% 0.731 0.726 0.723 0.719 0.710 0.702 0.693 0.688 | 0.5 
D:0) | 2.40 © 2.03 1:91" 1-79" 1.63 4.52) “1 -40mieiegs 1 
hence p:jy| 1.33 1.245 1.215 1.18 ° 1.14 1.11 - 1.08 1.07 1 
acalc.| 0.381 0.356 0.348 0.338 0.326 0.318 0.309 0.306 | 0.286 
afound| 0.394 0.373 0.366 0.358 0.347 0. 39 0.329 0.325 | (0.305) 


The values 8:8, =6:6, have been calculated from the tables of 
§ 16, viz. from those for y=0,75 and y=0,70. We have inter- 
polated for the values of y given in the above table. On an average 
the found values of 8 are 6°/, higher than the values ealeulated 
from our formula (30). If 8, = 0,30° were taken instead of 0,28°, 
the agreement would have been perfect. In connection with this it 
is remarkable that the dzjference between Bround ANd Beale, AaMounts 
almost constantly to 0,018 or 0,019. The course of the §-values is 
therefore perfectly identical with the course calculated from our 
formula; identity in the numerical values may be obtained by simple 
change of B, from 0,28° to 0,30°. 


459 


In fact, something is~ to be said in favour of this. In § 17 we 
namely calculated the value of @, from 2y = 6;:b,= &;: ?,, so 
that &, = &,: 27 = 0,429:1,5 became = 0,286. But in this it is 
assumed that the direction of the straight diameter remains the same 
down to the absolute zero point — which (as we already observed 
at the conclusion of § 14 (III p. 1051) cannot be the ease. On the 
contrary the coefficient of direction will approach to about 0,5 for 
all substances at low temperatures. It follows from this that the 
value of the liquid density at 7 =O, viz. @,, which is extrapolated 
from the direction of the so-called straight diameter (at the critical 
poit), will always be too great, hence v, too small, and also 6, =v, 
too small. Accordingly also the value of ?, = 6,: vz will be found 
too smali, when the inadmissible extrapolation is performed. 

The real value of &,, occurring in our formula (30) for b= /(v), 
will therefore be always greater than that which occurs in our 
relations found in I (which are valid aé the critical temperature). 
For the calculations of the real ,, in order to test our formula 
(30) by the observations, the calculation from &, = &,: 2; (which 
is based on this extrapolation) has therefore to be rejected. 

The above table need, therefore, give no occasion to conclude to 
any deviation with respect to the calculated and the found values 
of &; the more so as the course is perfectly the same, in consequence 
of the fact that in the relation (80) not 6, but b—b, occurs, so that 
through simple increase of 2 to 0,305 the found values of b—d,, 
resp. B—, will agree perfectly with the values of 8— 3, calculated 


. 


from our formula. 


Remark. We saw that the found values of 3, from the unsaturated 
gas state (§ 17) were all found too great for values of m>1; for 
values of m< 1 all too small i.e. larger or smaller than the values 
of p, or By caleulated from our formulae. Also in the region of 
coexistence (7 << 1) we found values for 3, which are all too small, 
nay even negative, hence impossible. Now the too small values may 
be easily accounted for either by association in the vapour at low 
temperatures, or through a faulty method of calculation of 8, from 
the law of Boynr (see above). But the too large values of By at 
m > 1 cannot be aecounted for in this way. 

It is, however, remarkable, that those too large values of 3, at 
m<c1, combined with the Uquid values at m< 1, seem to obey 
the relation 


B=0,4Vm 


pretty well, as appears from the table on the next page. 


460 


m= 1.95 1.43 1.13 1.04 1.01 | 0.98 0.94 0.91 0.88 0.81 0.74 8.65 0.60 
Vm= 1.40 1.20 1.06 1.02 1.005 | 0.99 0.97 0.954 0.94 0.90 0.86 0.806 0.775 


0.4 V\m= 0.56 0.48 0.42 0.41 0.40 0.40 0.39 0.38 0.38 0.36 0.34 0.32 0.31 
| 


8 found 0.55 0.51 0.45 0.43 0.42 | 0.39 0.37 0.37 0.36 0.35 0.34 0.33 0.325 


The values on the lefthand side of the dividing line might have 
a somewhat higher factor, viz. 0,42; those on the righthand side of 
the line (the liquid values) a somewhat smaller factor, e. g. 0,39, 

Yet this relation can hardly satisfy for several reasons. First because 
the formula ~=0,4’m would yield too large values of p, for 
larger values of m; it is at least inconceivable that the increase of 
6, with the temperature will continue indefinitely. But secondly the 
variability with v would disappear through this consideration, and 
only dependence on 7’ would be assumed. It would then be quite 
indifferent, whether 6 was considered at large or at very small 
volumes. That this, however, is entirely impossible, is at onee seen 
when we bear in mind that only by the assumption 6= /(v) we 
duly get r<3, s>*/,, and /’ >4! Only for “ideal” substances, 
i.e. at the absolute zero point, can ) be independent of the volume. 

Other relations could’ also be derived, among others between the 
found values of 8, 2—p, and m'‘), but they may also be due to 
chance. We shall, therefore, no longer dwell upon them. 


19. The characteristic function. 

It is known that for “ordinary” substances the value of the 
ee Pettey aa : 

characteristic” function @, 1. e. 


j—1 «¢ 
iS = 
4 fi-—l1 did. 
; é . m d&cocx. 
in which #=— —— is not constantly = 1 — as would have to 


e dm 

be the case, when a or } should either not depend on 7’ or only 
linearly — but with diminishing m inereases from 1 to about 1,4 
at m=0,6, with about 1,5 as probable limiting value when m 
approaches to 0. See vAN pEk Waars, and also my Paper in These 
Proc. of 25 April 1912, p. 1099—1101, in which it appeared that 
g~ =1-+ 6,8 (1—m) can be put in the neighbourhood of the eritical 
point. (loc. eit. p. 1101). 


1) When e.g. in the region of coexistence for the different values of m we write 
the corresponding values of n and n— f, 


viz. +0,23. 


i 
a appears to be about constant, 


461 


bavin¢ a 
For this it is however required that either —{ — ] = 6,8, or 
Om? \ an) i 


O20 : 
== {= | 6,9. (Cf. These Proc. of 3 Sept. 1913; p.56 and 57). 
Om? \ by. / 7. 


It is now certainly interesting fo consider how this will be for a 
substance as Argon, where yz is not 0,9, but 0,75. 

For the calculation of the values of / I bad to make use of 
RanktnE—Posr’s interpolation formula drawn up by Crommenin and 
treated already above (§ 18). This gives, indeed, the much too low 
value 5,628 instead of 6 for /;,, but 'as also the following values of 
J will possibly be too small in the same degree, there is a chance 
that the value of the ratio (f—1):(/,;—1) will not differ too 
much from reality. We then find the following table. 


| 
147.92 | 0.9819 | 0.8047 | 0.8103 | 1.104 | 5.696 | 1.015 
141.55 | 0.9396 | 0.6964 | 0.6311 | 
137.58 | 0.9132 | 0.5890 | 0.5529 | 1.965 | 5.987 | 1.078 | 1.15 
132.89 | 0.8821 | 0.4757 | 0.4609 | 1.032 | 6.137 | 1.110 | 1.15 
122.33 | 0.8120 | 0.2832 | 0.4742 | 1.033 | 6.534 | 1.196 | 1.24 
111.86 | 0.7425 | 0.1549 | 0.1618 | 0.957 | 7.047 | 1.307 | 1.25 
97.70 | 0.6485 | 0.0552 | 0.0685 | 0.805 | 8.080 | 1.530 | 1.23 
89.94 | 0.5970 | 0.0274 | 0.0391 | 0.702 | 8.945 | 1.717 | 1.21 


It is certainly remarkable that it would follow from the found 


04 : 
values of g that here too 4 would be about — 7, just as for 
me) I. 


Og 
ordinary substances as Fluorbenzene e.g. (see above). For (5 = 
k 


2) 
= — ee = — 6,63 (whereas it is — 6,8 for C,H,F). But on this 
head little can be said with certainty, as we have too few observations 
in the immediate neighbourhood of 77, at our disposal. 
The limiting value for m—0,6 is now, however, much lower, 
namely about 1,23 against 1,41 for ordinary substances. Now for 


462 


C,H,F the value of yz, is = 0,95; hence 0,:b, = 2Y~ = 1,90, and 
(6, : 6. )e = 1,90 <1,06 = 2:01,> whereas) 72,01 — 1,42. Further for 
Argon k= 0,75, hence 0: 6,=1,50 and (6,:5,),=1,49 X 1,018 
(See II, p. 986) = 1,516, whereas 1,516 =1,231. 

It follows from this that with great accuracy 


9, =V bo: be = V By 2 sw ee. DD) 


may be written for the limiting value at low temperature of the 
characteristic function ¢. 

It is therefore again only for “ideal” substances (6 = const.) that 
(> = 1, and hence ¢ continully =1 from 7% (then = 0) to the 
absolute zero. but for all the other substances the value of gy will 
increase from 1 to a limiting value, which will depend on the 
degree of variability of 6. 

As according to (36) (b,—d,),: 6, = 2y’ — 1 = 0,041 V 7; (see IIL 
§ 15), we have also : 

G, = VIS 004A ss 

We shall not enter any further into this subject, leaving it for a 
possible later discussion. 

In conclusion we shall just repeat what we have already remarked 
in I, p. 820, that the temperature dependence at extremely low 
temperatures, where the departures from the equipartition law make 
themselves felt, undergo a modification. But we shall not enter into 
this any further either, and we only mention that for Argon the 
departures from the said law fall entirely within the errors of ob- 
servation even at 90° absolute (the lowest temperature at which 
observations have been made). Besides, at those extremely low tem- 
peratures all substances will probably have passed into the solid 
state, and this state is controlled by other laws than the liquid and 
the gaseous state, for which our considerations exclusively hold. 


20. Conclusion. Though there are still many questions to be 
answered, and many difficulties left, we may already conclude in 
virtue of the foregoing to this: 

1. The quantity a of van per Waats’ equation of state seems 
within a large range not to depend on the density, so that the 


: a é 
molecular attraction can be represented by —, both in the gaseous 
y? 


and in the liquid state. *). 


1) Cf. also the conclusions in a paper by Tyrer in the just published number 
of the Zeitschr. f. Ph. Ch. (87, Heft 2) p. 198. 


463 


2. Whether the quantity @ is also independent of the tempe- 
rature, cannot be stated with perfect certainty yet. For as I think 
I have fully set forth in my Communieations of These Proce. of 25 
April 1912 (p. 1091 —1106) and particularly of 3 Sept. 1913 (44—59 , 


ae ; (One ; 0° 
the assumption of a darge value either of { — ] or of — 
k k 


or OL 
(see p. 56—57 loc. cit.) is necessary for the explanation of the 
course of the characteristic function g (see §19). And as, aceord- 


ing to the above, 6, is, indeed, variable with the temperature, but 
2 


probably not so much that —(r) gets the required value, besides 
t~/) i 


6 possibly also @ might depend on the temperature. Only a separate 
investigation ean furnish certainty about this. 

3. The quantity 4 depends both on v and on 7. The way in 
which 4 depends on v — which is expressed by a formula of the 
form (see I] p. 981 et seq., Ill p. 1048, formula (29)]| 


= j) xv y 
peel oie ; 
b,—b, Zi, 


in which «= (b—4,):(v—yv,), and n depends on the quantity y, 
which is in connection with 4,:4, — leads us to suspect that the 
variability of 6 is possibly chiefly a real change after all, caused 
by the action of the pressure p+ “/.2 and of the temperature, in an 
analogous way to that which van Der Waats had in mind when 


drawing up his “equation of state of the molecule’, with which the 

above expression shows a close resemblance. [ef. also I p. 980—-931 

(23 April 1914)|. Particularly also with regard to the temperatare 

dependence, viz. [see HI p. 1051—1058, formulae (85) to (36)| 
b,—b 


7 _* — 9y'_] — 0,047, 


this agreement is remarkable. But whereas vAN per WaAAtLs’ two 


exponents are different, our two exponents are the same and 
dependent on 7, i.e. on 7 so that m can vary from 3'/, (for y = 1) 


to © (for y='/,, ite. T=0), as has been set forth in II, p. 935. 

4. It seems to be unnecessary to ascribe the change of / to “quasi 
association’. It might namely be assumed that the complex mole- 
cules possess another volume than the simple ones, and from this a 
relation b= /(v) might be calculated — according to the known 
thermodynamic relations which indicate the degree of complexity as 
function of v and 7. R7'is then however multiplied by another factor 
which depends on the degree of association. 

What van ver Waats has treated in that sense on p. 1076 of 


464 


his Paper in These Proc. of 25 Jan. 1913 (published March 13%), 
had then already been treated very fully in a series of four papers, 
written by me at Clarens 1911—1912 (On the variability of / ete. ; 
see These Proc. of 26 Oct., 22 Nov. 1911; 24 Jan., 22 Febr. 1912). 
That a good deal may be attained in this way can sufficiently appear 
from these Papers. That difficulties present themselves of the same 
nature as have been advanced by van perk Waats on p. 1076 at the 
bottom (loc. cit.), has also appeared at the end of the 4 Paper 
(p. 716 et seq.). 

In any case it is a kind of relief that according to all that proceeds 
the assumption of quasi association does not seem absolutely necessary. 
The change namely of 4 with v and 7’ can very well be explained 
by other influences. 

5. That 6, gradually decreases with the temperature, so that b, 
would coincide with 6, at Z’—0, and accordingly the variability of 


4 would have quite disappeared — in consequence of which we 
approach more and more to the ¢dea/ equation of state with constant 
4, on approaching the absolute zero — this points to the invalidity 


of the kinetic assumption, that for very large volume (for b, only 
refers to /arge volumes) i.e. in ideal gas state, b, would be = 46,. 
For according to the well known kinetic derivation, 6, would then 
still be = 46, at the lowest temperatures, whereas it has clearly 
appeared that 4, approaches more and more to }, at low tempera- 
tures. Compare particularly Ill p. 1051, formula (85) and the sub- 
sequent eloquent table. 

6. Thus after all it would prove true what I wrote in I p. 809 
(These Proc. of 26 March 1914), that namely in v—é the quantity 
6 always refers to the real volume of the molecules m and is not 
= 4m, as the kinetic theory would lead us to assume. And in this 
way the difficulty, which I emphatically pointed out in II, p. 925 
(at the bottom)—926, would have naturally vanished. 

So it is getting more and more probable that the so-called quasi 
diminution of 4 does not exist, and that there remains only real 
diminution, which is represented by a formula of the form (29), as 
far as the dependence on v is concerned, and by a formula of the 
form (36), as far as the dependence on 7’ is concerned. 

Why the earlier kinetic assumption 6, = 4m is really a fiction, 
and what circumstance has been overlooked then — this I shall 
demonstrate in a separate Communication. 

It will then have become clear that only v—m, and not v—4in 
determines the thermic pressure -- which becomes already probable 
when the kinetic energy of the moving molecules is thought to be 


465 


uniformly absorbed by the surrounding medium (see p. 809 of I, 
already cited above). 

7. Hence at bottom the whole thermic behaviour of a substance 
does not depend on/y on the two quantities @ and 6, which deter- 
mine the critical quantities, which in their turn govern the law of 
the corresponding states — in such a way that all the substances 
behave correspondingly when they are only considered in equal 
multiples or sub-divisions of their critical temperature and critical 
pressure, but also (and the deviations from the said law are governed 
by this) on the absolute height of the temperature, at which the 
substance is considered. According to (86) every substance passes 
namely through the different types — characterised by the variable 
ratio b,:,, from the type of the “ordinary” substances, where 
i b, is about 1,8 (y= 0,9) to the type of the ‘ideal’ substances, 
where },is—=06, (y='/,) — when we descend from the ordinary 
temperatures to the absolute zero point (see the tables in I, p. 819 
and III p. 1052). 

The individuality of the different substances, which they continue 
to preserve within the region of the Law of the Corresponding States, 
is therefore entirely determined by the rea/ height of the (absolute) 
temperature. 

Hydrogen at 328° absolute (77’=107%) will e.g. on the whole 
(Law of Corresponding States) exhibit the same behaviour as Helium 
at 52° absolute (7’ also = 107%) — but H, will show a value of 
about 1,7 for the ratio 6,:4, at that higher temperature, while He 
at the same “corresponding” temperature shows a value of about 
1,2 for that ratio. 

For ve: hr we shall find about 2,7 for Hydrogen and Helium at 
their critical temperatnre, while vz: 6, = 2,1 is found for an ordinary 
substance at its critical temperature. Ete. Ete. 

And this may suffice for the present. I hope to come back to 
some separate problems later on, which are still awaiting solution. 
I may mention: the temperature dependence of / (see I, p. 811), 
the change of direction of the “straight” diameter from 77, to very 
low temperatures (III p. 1051), the form of the vapour-pressure 
equation p= 7(7'), the dependence of the densities of liquid and 
vapour on the temperature (in connection with the problem of the 
direction of the straight diameter); and finally the course of the 
characteristic function in its dependence on 7. 

But the very first point that will be elucidated in a following 
Paper is the circumstance mentioned under 6 of the conclusions, 
that 4, cannot possibly be = 4m. 

Fontanivent sur Clarens, April 1914. 


(September 26, 1914.) 


ons 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 
of Saturday September 26, 1914. 
Vout. XVII. 


DGC = . 


President: Prof. H. A. Lorentz. 
Secretary: Prof. P. Zeeman. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 26 September 1914, Di. XXIII). 


(SSyany Bwaa AN, PRISE 


H. vu Bots: “Modern electromagnets, especially for surgical and metallurgic practice”, p. 468. 

A. Wicumann: “On the Tin of the island of Flores”, p. 474. 

M. J. van Uven: “The theory of the combination of observations and the determination of 
the precision, illustrated by means of vectors.’ (Communicated by Prof. W. Karrryy), 
p- 490. 

H. Kameriincu Onnes and G. Horsr: “On the measurement of very low temperatures. XXIV. 
The hydrogen and helium thermometers of constant volume, down to the freezing—point 
of hydrogen compared with each other, and with the platinum-resistance thermometer,” 
p. 501. E 

H. Kameriincu Onnes and G. Horsr: “On the electrical resistance of pure metals ete. 1X. 
The resistance of mercury, tin, cadmium, constantin and mapganin dowa to temperatures, 
obtainable with liquid hydrogen and with liquid helinm at its boiling point,” p. 508. 

H. Kamertiscn Onnes: “Further experiments with liquid heliam. L. The persistence of 
currents without electro-motive force in supra conducting cireuits’, p. 514. 

Hl. Kameriincu Onnes and K, Hor: “Further experiments with liquid helium N. Harr-effeet 
and the change of resistance in a magnetic field. X. Measurements on cudmiam, graphite, 
gold, silver, bismuth, lead, tin and nickel, at hydrogen- and helium-temperatures.” p. 520, 

H. Kameruingu Onnes and H, A. Kuyrers: “Measurements on the capillarity of liquid 
hydrogen,” p. 528. 

F, A. H. Scurememakers and Miss W. C. bE Baat: “The system: Copper sulphate, copper 
chlorid, potassium sulphate, potassium chlorid and water at 30°, p. 533. 

J. Borsexen: “The Catalyse.” (Communicated by Prof. A. F. Hlotteman), p. 546. 

F. M. Jagger: “Researches on the Temperature-coefficients of the free Surface-energy 
of Liquids between —80° to 1650° C. Vil. The specilic surface-energy of the molten 
Halogenides of the Alcali-metals”. p. 555. “Ibid VIL. The Specific Surface-energy of 
some Salts of the Alcali-metals’’, (Communicated by Prof. H. HaGa). p. 571. 

G. pe Brur: “A crystallized compound of isoprene with sulphur dioxide.” (Communicated 
by Prof. P. van Rompurcn), p. 585. 

J. P. van per Srox: “The treatment of frequencies of directed quantities. p. 586. 

J. J. van Laar: “Some remarks on the values of the critical quantities in case of asso- 
ciation.” (Communicated by Prof. H. A. Lorentz), p. 598. 

J. J. van Laar: “On apparent thermodynamic discontinuities, in connection with the value 
of the quantity J for infinitely large volume.” (Communicated by Prof. H. A. Lorenrz), 
p- 606. 

H. R. Kroyr: “Current Potentials of Electrolyte solutions.” (Communicated by Prof. Ernxsr 
Couen), p. 615. 

Hi. R. Kruyr: “Electric charge and*limit value of Colloids,” (Communicated by Prof Ernsy 
COHEN), p. 623. 


ol 
Proceedings Royal Acad. Amsterdam. Vol. XVIL. 


468 


Physics. — “Modern electromagnets, especially for surgical and 
metallurgic practice.’ By H. pu Bois. (Communication from 
the Bosscua-Laboratory). 


(Communicated in the meeting of May 30, 1914). 


Carrying-Magnets. The lifting-power of the famous steel magnets 
of Logrman and van WertrrEN, has for a long time belonged to the 
somewhat antiquated subjects. However, traction-electromagnets are 
now being much more used in different forms, especially for loading 
and transportation purposes. 

In general we may say, that for sueh magnets with armatures at 
a very small distance Maxwetw’s well-known law holds; accordingly 
B*/8Sa measures the carrying-power per unit cross-section of an 
almost closed magnetic circuit. Prof. TayLtor Jonus has entirely 
confirmed this by experiment in the Bosscua-Laboratory. The mag- 
netic balance as a measuring instrument is equally based upon this 
fundamental law. Electro-magnetic brakes on this principle are also 
being more and more used. 


Field-Magnets are of more interest for a variety of scientific and 
practical purposes. In these Proceedings a description was given of 
semicircular magnets’), one of which, weighing 350 kg., with an 
interferrum of 3 0,5 mm. gave a uniform field of 59 Kilogauss, 
while using only a few Kilowatts. With a cryomagnetic “immersion- 
armature’ in a liquid gas at low temperature this reduces to 45 
Kilogauss. With the heaviest type weighing four times more (1400 kg.) 
we may cet. par. expect no larger increase than 10°/, , thus reaching 
65 and 50 Kilogauss respectively. Until now these field values have 
not been superseded, no more than the Haarlem magnets were. 
For the investigation of several highly interesting problems they are 
absolutely necessary. 

With regard to so small a rise of the field however it requires 
dne consideration whether a further increase of the size of the magnets 
appears justifiable. For while the weight increases as the third power 
of the limear dimension, thus becoming quite unwieldy, the field 
rises logarithmically only, which means a great disadvantage. In fact 
for a given field we practically obtain only a larger interferrum. 
However convenient this may be, it is questionable whether it justifies 
the very high expense which gradually begins to surpass an average 
laboratory-budget. 


1) H. pu Bors, These Proceedings 12 p. 189, 1909; 13 p. 386, 1910. 


469 


The results mentioned are partly due to concentration of the 
Ampere-turns near the air-gap and also to careful calculation and 
design of all details; the theory of polar armatures ') communicated 
to the Academy, contributed its share to the result. 


Intestinal magnets. Incidentically the formulae for attractory arma- 
tures were also given in the paper referred to. They show, that the 
attraction of saturated ferromagnetic particles is a maximum for cones 
with a semi-angle of 39°14’, and for prisms of 30°; for non- 
saturated ferromagnetic or for paramagnetic substances these angles 
are 42°11’, and 32°8’ respectively. According to the principle of 
Farapay and Kervin the attraction is determined by the gradient of 
the first [second] power of the intensity 9 of the field for the first 
[second] group of substances. 

Some time ago Prof. Payr*) proposed a magnetic diagnosis, 
prophylaxis and cure of peritoneal adhesions and similar deviations. 
For this purpose a ferromagnetic intestinal filling is introduced either 
per os or per rectum. Then magnetic force is applied from outside 
without the necessity of more or less dangerous laparotomy. At the 
request of this well-known surgeon I was glad to collaborate in the 
attempt towards a practical solution of this peculiar a¢traction-problem ; 
for a rational treatment of it the above-mentioned armature-theory is 
absolutely necessary. The existence of an indifferent intermediate 
zone and the necessity for exciting large attractive forces only beyond 
this, characterizes this particular question. 

The ordinary type has a core of high permeability (of 12 cm. 
thickness and 40 em. length). It is somewhat concave at one end and 
thus fits the average form of the human body. In the paper referred 
to the formula is given for 9, 05/dr and 0?.9/dx? on the «x-axis 
for the case of a segmental spherical armature and for that of a 
coneave paraboloid of revolution. For the latter case it was shown 
that a certain distance not before a maximum of the field was reached. 
In this “neutral” point the gradient is zero and therefore the attraction 
also vanishes; the latter then increases, reaches a maximum and de- 
creases again gradually. This distribution of the field is favoured by 
the higher magnetisation at the periphery of the core compared with 
that of the centre, which makes this case similar to that of hollow 
cores. In the outset I even used a core with a conical bore in 
order to allow an eventual radiologic transmission through it; this 
however proved later on to be practically unnecessary. A central 


a) H. vu Bois, These Proceedings 15 p. 330, 1912. 
*) E. Payr, Miinch. med. Wochenschr. 60 p. 2601, 1913. 
31* 


+70 


filling of the core with a substance of higher permeability might be 
made -to compensate the distribution of the field above described. - 
In our case however this very topography of the field is desired ; 
for it is within the peritoneum only and not in the surrounding 
layer (the thickness of which individually varies from 2 em. to 10 em. 
and even more) that an attraction may be usefully exerted. Towards 
its other end the core gradually becomes thicker and the end is 
formed by a flange in order to decrease the magnetic reluctance ; 
the counter-action of this pole compared with the attraction of the 
working pole is negligeable. 

The coils are wound with enamelled copper wire or with oxydized 
square aluminium wire the thickness of which increases by steps 
from the working pole towards the other end. This principle is 
well-known for galvanometers and has also found partial application 
in my semicircular magnets. The increased efficiency of the “polar 
windings” must necessarily cause a greater heating effect which may be 
counter-acted by water circulation. ; 

Until now this precaution proved unnecessary, the more so because 
too cold iron may cause undesirable vasomotoric reflexes of the 
patient. The front flange of the coils is conical, in order not to be 
in the way of the operator’s eyes and hands; it may be provided 
with a corrugated peripheric radiator. The use of alternating currents 
is not advisable; but a pulsating current may be caused by periodic 
short-circniting of the magnet, while a non-inductive resistance remains 
switched in the circuit. The relaxation-time is a few seconds; by 
exciting the polar coil only it may be diminished to a few tenths 
of a second; when pulsations are often to be applied, it is advisable 
to use a subdivided core. 

In order to reduce the weight as much as possible the core onght 
to be saturated only to */, or */,. A minimum total weight is 
obtained for a dimensional ratio’) between 3 and 4; then the power 
required is only little above its minimum value; it amounts at most 
to 4 K.-watt, for most operations it is considerably less; and con- 
sidering the short duration of an operation the energy consumed 
(K.-watt-hours) is but very small. The magnet weighs about 100 ke. 
and is suspended by a kind of crane above the operation table, in 
such a way that its 6 degrees of freedom may be disposed of, i. e. 
a displacement along the vertical and a rotation around it, and the 
same for two horizontal axes parallel to the body of the patient 
and normal to it. Below the patient the ROnrcEn-tube is placed, as 


1) Calculated from the demagnetizing factors for short cores, as measured by 
S. P. Taompson and E. W. Moss, Proc. Phys. Soc. Lond, 21, p. 622, 1909. 


471 


far as possible from the magnet, in order to diminish its deviating 
action on the cathode rays'). In some cases the patient may be 
treated while standing, which is much simpler. 

Deep-seated intestines (7—20 em. under the skin) are treated 
without pole-shoes. For those lying nearer the skin, the following 
pole-shoes are used which may be made of a highly saturated, 
polished and nickeled, substance, such as ferrocobalt. 

1. A “drawing-pole” in the form of a truncated cone with a semi- 
angle of 40°; the attraction is strongest in the apex of the cone. 
The contents of the intestines may be first drawn towards a par- 
ticular spot and then attracted towards the magnet. 

2. A prismatic pole with a semi-angle of 32° for the treatment 
of longer intestinal sections. 

3. An unsymmetric hoof-shaped “dragging-pole” for applying force 
parallel to the peritoneum. Starting from the above-mentioned principle 
it may be shown that a maximum gradient of §* is reached when 
the narrow pole front forms an angle « = 65°54’ = t7-1V5 with 
the direction of dragging. For a very long prism on the other hand 
it ought to be ¢ = 60° = tg—'!V3. In this way the best adapted shape 
of the pole-shoe may be determined, also fitting the cylindric core. 
For special purposes pole-shoes of various shapes may be designed. 

The forces used bere have often been measured with small iron 
test-spheres. The force component is 

3 ‘ 0 r 04° 
Iie = vi) ’ 

An Ou 2 Ox 
v denoting the volume, 7 the radius, there being no question of 
saturation. This expression is quite independent of the nature of the 
substance if only this is not too weakly ferromagnetic. The force, 


expressed as a multiple of the weight G of the ,test-sphere will be 
greater, the smaller the density of the latter. The value f,/G—=1 
corresponds to the case that at a certain distance under the magnet 
the sphere is just being prevented from falling down. Considering 
this, spheres were made of magnetite (/’,O, = ferroferrite = ferr. 
oxyd. oxydulat. nigrum.) which quite fulfilled my expectations. Best 
of all proved small spheres of 1 cm. diameter of /’,O,-powder 
mixed with a little mucilage and some light neutral powder; generally 


1) The Rénreen-tube is moved by the foot of the operator. The deviation of 
the cathode-current is proportional to its own strength, the value of the field at 
that place and the sine of the angle between these two directions; these three 
quantities onght to have low values. An iron-clad Réyreey-tube might prove useful ; 
but sparking constitutes rather a dilficully. In some cases a compensating coil 
near the cathode rays may be arranged. 


472 


these were used as test-spheres. This substance which fulfils all 
magnetic conditions is also to be recommended from a clinical point 
of view; it is neither poisonous nor soluble; it does not rust nor 
causes hydrogen to develop; it is not resorbed and hardly irritates 
the mucuous membrane. It gives good R6NTGEN-contrasts, even without 
addition of bismuth carbonate and it is more satisfactory than ferram 
reductum pulverisatum; it is the principal ingredient of the emulsions, 
which are given per os or per anum, the prescriptions of which 
vary in practice. On this point and on the very satisfactory surgical 
results I need hardly give full details. The following will suffice *). 

The operative conditions were fulfilled and even surpassed. The 
practice gained with a number of patients led towards a reliable 
diagnosis of the normal or abnormal mobility of the intestines and 
of adhesions and their exact place. It was often managed to stretch 
and to raise them carefully either in the stage of fibrous adherence 

hat of lasting mutual connexion. Of course reliable 

© ihe results cannot be obtained until later. The treatment 

day lave a great effect on the position of the intestines or of their 

special sections; such a locomotion highly influences the peristaltic 

function; this ought to be especially the case with pulsating magnetic 

fields of smaller or greater frequency up to about 10 or 20 per 
second and of different form of pulsation-curve. 

The accelarated or retarded displacement of intestinal substance 
containing ferromagnetic ingredients ; the dragging of this into organs, 
which are too deeply seated to be reached in any other way, especially 
the appendix, with a view to radiologic diagnosis, the turning and 
loosening of intestinal slings remain subjects for further research. 
The principal advantages of this method are its localisation on a 
special part of the intestines, the precise regulation of the displace- 
inent, the easy dosing of the effect by regulating pole distance and 
current and the simultaneous radiologic examination. : 

In order to determine the topography of the field for various distan- 
ces and currents, it was fixed by iron filings, with or without pole- 
‘oes und if necessary it was measured with a standardized test-coil. 

yuicing along the axis, from the start at the concave pole front 

uinimum of the field is first met, then a maximum. To these cor- 
respond theoretically a transverse maximum and minimum respecti- 
vely, and also an unstable and a stable zero-point of attraction. This is 
easily shown with a test-sphere in an axial glass tube, which is seen 
to remain suspended in that very point. With a plane pole front 
such singularities do not appear. 


) See also E. Payr, Ber. D. chirurg. Congress, Berlin April 1914. 


473 


The attraction of a number of test-spheres or pills was measured 
under different circumstances with a spring-balance; its maximum 
was found at a distance of 4—5 em. and amounts up to 25-fold 
weight; the greatest “carrying distance” is 22 cm., for test cylinders 
even more. For a round drawing-pole the maximum was found at 
2 or 3 cm. and reaches 50-fold weight; at distances greater than 
7 cm. the attraction becomes smaller than that observed without 
the use of a pole-shoe. The coils were constructed in such a way 
that their purely electrodynamie attraction, which is determined by 
the square of the current, contributes considerably to the total force. 
With a dragging-pole a transverse force is obtained up to 25-fold 
weight at a distance of 2,5 cm. 

Though for our purpose the type described proved amply sufficient, 
it appears however interesting to study the properties of a similarly 
enlarged or reduced instrument. If the linear dimensions be n-fold 
the weight of the iron varies as n’*, that of the copper as n* (or as 
n*, depending on the mode of winding), tle kilowatts consumed as 
n (or respectively as n*), the attraction of non-saturated particles at 
a given distance however nearly as 7‘. This 4° power (in fact 
about the 3,7") is evidently very favourable, especially as compared 
with the above-mentioned very uneconomical logarithmic progression 
for field-magnets. We may safely predict that it will be possible to 
produce any necessary force with magnets which do not yet become 
unmanageable and the cost of which will hardly prove a serious 
obstacle in this case, where life and health of the patients may be 
at stake. 


Extracting magnets. In this way it ought to be possible to move 
about ferromagnetic probes brought into the body on purpose or to 
extract undesirable objects, such as steel bullet shells, broken needles 
or injection-syringes and various iron or nickel objects, which are 
daily met with in the surgery of accidents. 

Also an effect on other organs, less soft than the intestines may 
be thought of. It has long been known that all tissues are diamagnetic; 
Faraday already showed that this is also the case with blood; the 
iron atoms in haemoglobine are bound in such a way that no para- 
magnetism occurs, no more than e.g. for potassium ferrocyanide. 
Picker’) showed that a magnet repels the red blood globules 
relatively to the serum. It is moreover also known that the flow of 
diamagnetic liquids through tubes and their dropping may be con- 


1) A. PLiicker, Pogg. Ann. 73 p. 576, 1848. 


A474 


siderably influenced under special circumstances by very strong 
fields *). 

By putting 2 <4 the effect of reducing the dimensions is at once 
evident; this is interesting with a view to the design of the usual 
ophtalmic magnets which may also be improved by the above caleu- 
lations and experiences; the maximum distance in this case is not 
more than 2,5 em. A type is now being made of 8,5 em. diameter 
of core, serving the double purpose of an intestinal magnet of less 
strength than the above and at the same time of a very powerful 
ophtalmiec electromagnet. 


Ore separators have long been applied in metallurgy to separate 
unmagnetic from ferromagnetic or only paramagnetic powdered ove 
by the dry or the wet method. These apparatus are variously con- 
structed; the principal magnetic organ is however essential and 
common to them all and is a more or less finely ribbed polar arma- 
inve. The best cross-section for a definite mean size of the grains 
may be determined by means of the theory above-mentioned for a 
prism semi-angle between 30° and 32°8’. 


Mineralogy. — “On the Tin of the Island of Flores.” By Prof. 
Dr. A. WicHMAnNn. 


(Communicated in the meeting of June 27, 1914). 


During the last decenniams very contradictory answers were given 
to the question regarding the occurrence of tin-ore in the Isl and 
of Flores. The fact that the solution of this question does not only 
regard the interests of a mining-scientifical nature, but is likewise 
very interesting from a mineralogical and geological point of view 
may justify the attempt of elucidating this subject. 

In ihe first place we have to bring into remembrance the fact, 
that in the Sunda Islands the older geological formations gradually 
disappear if we move in that range of islands in an_ easterly 
direction, till — beginning from Bali — only neogenie and _pleisto- 
cenic sediments are found, and at the same time tertiary and _post- 
fertiary eruptive rocks with their tufas begin to play a predominant 
part. The question rises then: Does Flores make an exception to 
‘iis rule and do we find in this island remains of ancient granite 
siocks, accompanied by deposits of tin, or are all the reports regarding 
the occurrence of this ore only of a legendary nature ? 


1) QO. Lresknecut and A. P. Witts, Ann. d. Phys. 1 p. 183, 1900. W. J. pp Haas 
and P. Drapier, Ann, d Phys. 42 p. 677, 1915. 


475 


The first report originates from J. P. Freyss, who wrote on account 
of his information received in 1856 in Manggarai (West Flores). 
“In the mountains of Rokka at Sui Tui’) gold is found, whilst 
“Mount Aspana produces tin)”. 

In 1866 a resolution was taken by the Governor General L. A. 
J. W. Baron Storer van ps Berrie “to send a trustworthy funetionary 
“to the isle of Flores in order to investigate if on the south-coast 
“of this island in the neighbourhood of the village of Rokka tin 
“is found”. It is unknown whether the resolution (of January the 
15 N°. 3) was ever put into execution *). 

Five years afterwards J. A. vAN per Cus fixed the attention to 
the fact, ‘‘that every year a rather considerable quantity of arm- 
“and leg-rings made of tin and of a rude construction was exported 
“from the district of Rokka, situated on the south-coast of the isle 
“of Flores’ *). The Indian Government having been requested to 
order the controller S$. Roos, established in the isle of Sumba, to 
make an investigation whether in reality tin occurred in Flores, a 
resolution was taken to this effect November the 13! 1871 N°. 3, 
and the Board of Directors of the Soeiety of Industry and Agricul- 
ture received a short time after from the above-mentioned functionary 
“a few specimens of tin-ore from Masara’. 

According to the investigation which was entrusted to C. br 
GaveERE, the mineral in question was pyrites*). In the mean time 
the Governor General Piwrer Mier had authorised, by resolution 
of April the 18% 1872 N°. 59, the resident of Timor to send an 
expert to Rokka “that he might convince bimself on the spot, in 
“how far tin-ore is dug up and melted there, and at the same time 
“to collect some specimens of ore and rocks” °). This investigation 
had neither any result, for, as was reported, the native chief’) — 
this was the expert — “had until now, on account of ill health and 

1) The place is called Sui (manggaraish) or Tui (endehneish) and is situated on 
the west-side of the Aiméré bay. There can be no question of the occurrence of 
gold there, for behind that place rises the extinct vuleano Komba. 

2) Reizen naar Mangarai en Lombok in 1854—56. Vydschr. voor Ind. Taal-, 
Land- en Volkenkunde. 9. Batavia 1860, p. 507. 

*) Koloniaal Verslag van 181, p. 29. 

4) Tijdschr. voor Nijverheid en Landbouw in Ned. Ind. 16. Batavia 1871, p. 
158-159. 

5) Tydschrift voor Nijverheid en Landbouw in Ned. Ind. 17. Batavia 1572, p. 184. 
21. 1877, p. 40—41. 

6) As quoted 17. 1872, p. 385. 

7) He proved afterwards to be an Arab who had settled in Sumba. (Koloniaal 
Verslag van 1591, p. 22). 


476 


“the unfavourable disposition of the population of the island, not 
“vet fulfilled the order given to him. ’) 

A short time after 5. Roos communicated the following inform- 
ation concerning tin. “The people of Rokka often sell on the shore 
“bracelets made of tin, but they do not allow anybody to visit 
“their village... The Endehnese admit as rather certain that much 
“tin-ore oceurs in the ground of Rokka, but for fear of being mur- 
“dered they dare not venture into this village; this was likewise 
“the reason why nobody, even for ample payment, would accom- 
“pany me thither, so that I had to desist from the journey: It is 
“however known to me that proas of Endeh and likewise Chinese 
“of Kupang and persons of other places from time to time come 
“there to trade with the natives i.e. they anchor at Wai Wau or 
“at Aimeré and carry on their trade on the shore with the people 
“of Mangarai and with the inhabitants of the mountains, the latter 
“offering for sale a trifle e.g. a parang or a pair of bracelets made 
“of tin to the merchants. The bracelets are heavy, of rude work- 
“manship, more than a hand broad and are worn above the elbow.” ?) 
According to J. G. F. Riepen the tin is collected in Liu and Langgi 
(read Langga) by the natives ‘fin a mysterious manner.” *) 

Hitherto there had only been question of the supposed occurrence 
of tin in the district of Rokka, but in 1877 F. C. Hnynen wrote : 
“according to reliable reperts a considerable quantity of tin is found 
“in the territory of the Rajah of Larantuka, somewhere in Flores... 
“the tin objects resembling silver gave lately to a traveller whom 
“we met in Flores, the conviction, that the tin there is of an excel- 
“lent quality.” *) 

A request made by L. P. pen Dekknr d.d. Kupang July 1s* 1882, 
but not granted, to obtain the permission of prospecting in Flores, 
tbe Solor and the Alor Islands fixed again the attention of Govern- 
went to the tin. The mandate of trying to obtain, if possible, some 

1) Verslag omtrent het Miynwezen in Ned. Indié voor het jaar 1872. Jaarboek 
van het Minw. in Ned. Indié. Amsterdam 1873. I, p. 327. — Koloniaal Verslag 
over 1873, p. 260. — Two years afterwards it was reported however that, on 
account of the distrust of the population, it could not be ascertained whether the 
territory of Rokka was really rich in tin. (Koloniaal Verslag van 1875, p. 26). 

*) lets over Endeh. Tijdschr. voor Ind. T. L. en Vk. 24. Batavia 1877, p. 515. 

8) The island cf Flores or Pulau Bunga [sic.!]. Revue coloniale internationale 1. 
Amsterdam 1886, p. 66. 

4) Het ryk van Larantoeka op het eiland Flores. Studién op Godsdienstig, 
Wetenschappelik en Letterkundig Gebied. 8, No. 6. ’s Hertogenbosch 1876, p.34—35. 
A. JAcoBSEN described tin bracelets of East Flores (Reise in die Inselwelt des 
Banda-Meeres. Berlin 1896, p. 606—61). 


477 


of the tin objects originating from Rokka, given to the resident of 
Timor and to the magistrate of Larantuka was complied with. *) 

From the investigation made by H. Crermr it appeared that a 
tin bracelet contained lead, whilst a specimen of tin-ore was very 
ferruginous. *) 

The examination of some bullets led further to the result that they 
were not composed of tin, but chiefly of lead and zine with traces 
of tin, copper and iron. Should the “strongly ferruginous” ore be 
identical with the specimen “stroomtinerts van Oost-Flores”, mentioned 
in the catalogue of the Mineralogical Collection of the Office of the 
Department of Mines at Batavia under N°. 3302 and really contain 
tin, then it is certainly not originating from this territory, where in 
several places titaniferous iron-ore but no tin is found. 

In consequence of the resolution of the Governor General O. van Rens 
of August the 5 1887 N°. + the resident of Timor was authorised 
to order the magistrate E. F. Kurran to go to the district of 
Rokka, situated on the south-coast of this island, in order to obtain 
reliable evidence about the occurrence of grounds containing tin-ore 
in the interior of the isle of Flores.*) Kieran had supposed that he 
would reach his aim by choosing as place of issue the village of 
Nanga Lian in the district of Toa *) situated on the north-coast, where 
he landed the 12 of September. The 17 he marched to Nbai *) 
(about 8°34’ S., 121°10’ E.), he was however decidedly refused to 
go further to Soa and Poma, the supposed finding-places of the 
tin-ore. An inhabitant of the mountain of the village of Dora told, 
that at a few days’ walk distance in a place called Watam Kadjan, 
situated between Poma and Soa, specimens of native tin were collected 
in the ravines, when the rainy season was over, to make bracelets 
and other ornaments. After having returned to the coast on the 
19% he continued his journey as far as Rium on the 20. The 
Rajah here, however, did not know anything about tin, nor was he 
inclined to procure an interpreter or a guide for the journey to the 
interior. Without having attained his end Kian returned home again 
to Kupang. 

1) Verslag van het Mijnwezen in Ned.-Indié over het jaar 1882—83. Jaarboek 
van het Minwezen in Ned.-Ind. 12. 1884. Techn. en administr, ged, p. 376, 304. 

2) Bydragen uit het scheikundig laboratorium van het hoofdbureau van het Mijn- 
wezen. Jaarboek van het Mijnw. 13. 1884. Wetensch. ged., p. 312. 

3) Koloniaal Verslag van 1891, p. 23. 

4) He had already paid a visit to this district in 1875. (en voetreis over het 
oostelijk deel van Flores. Tijdschr. v. Ind. T. L. en Vk. 34. 1891, p. 530—582. 

5) Embai according to J. W. SroursEspuK.. 


478 


When in 1888 two applications for concession were made, one 
by A. Laneen, who had received from a Chinese a specimen of granite 
and likewise a specimen of tin-ore, said to be originating from “the 
river Aspana’, and a second by R. van pen Brorx') with 4 others, 
who requested to be allowed to explore 100000 bouws (!), the 
Governor General C. Prnakker Horpisk resolved to have an investigation 
made by an expert into the supposed abundance of tin-ore in Flores. 
By resolution of the 20 Sept. 1889 n°. 18 the mining-engineer of the 
Department of Mines C. J. van ScHEt.u was appointed leader of 
the expedition. Tie expedition left Batavia on the 15 Nov., and 
arrived the 30% next at Kupang. After the resident of Timor had 
ordered the magistrate E. F. Kieran to accompany the expedition, they 
left on the 3°¢ Dee. for Larantuka and afterwards to Endeh, where 
the assistant magistrate F. A. Broeman joined them. On the 10" they 
disembarked at Soa, situated on the westside of the Aiméré Bay, and 
a reconnoitring-expedition was undertaken in a north-eastern direction 
as far as the village of Foan, where however none of the inhabitants 
could be prevailed upon to accompany the expedition to Langga, 
“which village is said to be situated in the neighbourhood of the 
“tin-region”’. 

After their return. on the 11 December they went into bivouae 
which they left again on the 15%. After a 1O hours’ march in a 
north-eastern direction the mountain-ridge of Watu Loko was reached 
in the neighbourhood of Ekofeto. The next morning, a short time 
before their departure, they had to sustain an assault in which 
Van Scnette and Kieran were wounded by sword-thrusts. In a 
forced march the expedition drew back to the Aiméré Bay, which 
they left in the afternoon of the 17 to sail back to Kupang °). 

Krom the information he had obtained Van ScueLLE came to the 
couelusion “Ist that none of the Endehnese, who had visited the 
“eoast-region of Rokka and the neighbouring Mangarai knew anything 
“of an importation of tin under any form whatsever. 2°¢ that the 
“mountaineers of these regions with whom they came into contact 
“possess tin ornaments, and use likewise tin to make their fishing- 

1) This gentleman undertook in 1889 a scientifie journey by order of the Kon. 
Nederl. Aardrijkskundig Genootschap Tie results obtained have however never 
been published. 

2) Koloniaal Verslag van 1890, page 21. — Verslag van het Mijnwezen over het 
4e kwartaal 1889, p. 11. — J. CG. van Scusie. Verslag van het onderzoek 
paar het voorkomen van tinertshoudende gronden op Flores. Extra-Byvoegsel der 
Javasche Courant. Batavia 1890, No. 10. — Tijdschr. voor Nederlandsch-Indié 
1890. 2, p. 77 —79. — Tu. Posewrrz. Die niederliindisch-indische Zinnerzexpedition 
auf Flores. Das Ausland 64. Stuttgart 1891, p. 145—149. 


479 


“nets heavier; 3° that tin has little value for them and iron and 
“copper is valued higher by them; 4% that constantly as finding- 
“place of tin a special spot is indicated, situated northward from 
“Mount Roukka, and the natives possess there considerable quantities 
“of tin’ '). Further lhe asserted “that the idea formerly occasionally 
“suggested, that the tin that the people of Rokka possess, should 
“be imported or proceed from solder of petroleum- or other tins 
‘must be rejected as utterly unfounded”. 

The summary of his considerations was: ‘ As far as the information 
“I obtained reaches, | must admit that the soil to the north of the 
“Mountain of Rokka is very rich in tin-ore...... Along a fissure 
“running probably from East to West along the South-coast of 
“Flores, the volcanic products have found a way and partly covered 
“the other formations. The region containing tin-ore is situated at 
“the frontier of the two formations, and we must admit, that the 
“older formation there is strongly impregnated with tin-ore, and that 
“by the desaggregation this comes free at the surface’. 

The favourable expectations raised by VAN ScHELLE’s report 
induced the Indian Government to send out a second expedition this 
time however supported by a strong military power. (Resolution 
of the 31st March 1890) ’). 

On the 11 May 1890 a detachment departed from Surabaya and 
arrived on the 14 in the Aimeére Bay, where on the left bank of 
the Wai Moké (Aiméré River) a bivouae was pitched. On the 8" July 
the well-known Watu Loko was occupied. On the 24% and 25 under 
protection of a strong patrol C. J. van Scretie made from this 
place in an eastern and north-eastern direction reconnoitring excursions 
to the supposed tin-region. Instead of grounds containing ore he 
found however crater-mountains, of which Kopo Lebo and Lebi Sega 
were ascended. On the 29! the patrol reached the top of Wolo 
Meré, 1650 feet high, and discovered that, as far as could be seen, 
it was of a voleanic nature. 

Atter this complete failure a last effort was ventured to reach 
the ‘“tin-region” from the district of Toa situated on the north-coast, 
where E. F. Krein had taken information in 1887. By resolution 
of 10% Sept. 1890, N°. 1 it was stipulated that vAN ScHELLE and 


1) In reality more than a dozen places were mentioned. 

2) Koloniaal Verslag van 1870, page 22., 1891, p. 2329. — Verslag van het 
Mijnwezen over het 2de kwartaal 1890, p. 16; dde kw. 1899, p. 12. — P. G. 
ScumipHAmEer. De expeditie naar Zuid-Flores. Indisch Militair Tijdschrift. 24. 
Batavia—'s Gravenhage 1893, p. 101—115 %7—218, 289-307, 315—404, 
493—504, 25. 1894, p. 1—11. 


(tT to 
Wolorsfok / 
(o> 


PE INGASS 


5) 


his companions were to leave the south-coast, to repair to the 
district mentioned above. In the mean time a division had arrived 
there on the 26" September, that transported their head-quarters to 
Nbai on the 27" October. When van Scue.Le had been obliged to 
leave the spot on account of ill-health, he was replaced by the 
overseer A. F. H. Heusch and along the river Koli they marched 
into the interior towards Mundé, but on this expedition likewise 
only voleanic formations were found.*) Inereasing cases of illness 
rendered a longer residence impossible, so that on the 23'¢ of November 
Nbai and on the 2°* of December Remang had to be evacuated. *) 

In the mean time information about the oceurrence of tin was 
gathered from other sides. J. W. Merersure on his march across 
Manggarai in 1890 did not see anywhere an object made of tin; 
only at Nanga Mborong he obtained a tin bracelet, which was said 
to originate from Anduwa to the W. of Wai Moké, where, as was 
said, the tin-ore was to be found. *) In the beginning of 1891 the 
controller J. F. Horpr was sent to the North-coast of Flores, in 


1) According to P. G. ScHMIDHAMER Poré was the real finding-place of the tin 
(p. 404) and not Poma, Mundé and Soa (p. 500). 

*) Koloniaal Verslag van 1891, p. 26—29. — J. W. SroursEspiuK. Een mede- 
deeling over het eiland Flores. Tijdschr. K. Nederl. Aardr. Gen. (2) 8. 1891, p. 
748—749, map N°. IV. 

5) Dagboek van den controleur van Bima, J. W. MEERBURG, gehouden gedurende 
zijne reis door het binnenland van Manggarai. Tijdschr. y. Ind. T. L. en Vk. 36. 
Batavia 1893, p. 143, 148. 


48] 


consequence of a report of ALBerT CoLrs') according to which the 
inhabitants of Potta bring tin to market. That information was not 
confirmed by him, on the contrary he was told that in the district 
of Dua to the South of Potta, tin, gold and even diamonds occurred.’) 

The last investigation took place in the end during the years 1910 
and 1911 by J. J. Pannexork van Ruepen. In the second of his 
papers *) mentioned at the foot he says with regard to the occurrence 
of tin: ‘According to the reports of WichMann and VAN SCHELLE 
“there was sufficient foundation for the supposition that the tin that 
“was used by the population of Central Ngada was originating 
“from ore found in the district itself. *) As the presumable finding- 
“place the region to the North of voleano Inié Rié is indicated. On 
“the occasion of the expedition in North Ngada in 1890 a slight 
“quantity of fine cassiterite was collected near Torang. The investi- 
“gation L was charged with about the occurrence of tin-ore in these 
“regions could not yet be brought to an end on account of the un- 
“favourable political situation.” *) 

After the above historical explanation we shall now try to answer 
the question whether there is sufficient ground to admit that tin 
occurs in Flores. C.J. van Scuenie had answered the question affirm- 
atively and supported his answer by the 3 following hypotheses. 
1st. nothing is known about the importation of tin objects, 2°¢ the 


}) CoLFs made a journey through Manggarai in 1880. In the description of his 
journey not a single word is said about the above communication (Het Journaal 
van ALBERT Cours. Batavia 1888, p. 71—72). 

®) Verslag van de reis van den Controleur Horpt naar de noordkust van West- 
Flores. Tydschr. voor Ind. T. L. en Vk. 36. 1893, p. 281, 292. 

8) Eenige geologische gegevens omtrent het eiland Flores. Jaarbock van het 
Mijnwezen in Ned. Ind. 39. 1910. Batavia 1912. Verhandel. p. 132—138, pl. X. 
— Overzicht van de geographisclie en geologische gegevens verkregen bij de 
Minbouwkundig-geologische verkenning van het eiland Flores in 1910 en 1911. 
Jaarboek van het Mynwezen 40. 1911. Batavia 1913. Verhdlg., p. 208—226. 

4) This remark is, in so far as regards myself, entirely invented. The only 
thing ever wrilten by me about this subject runs as follows: “Ebenso schleier- 
“haft (namely, as the origin of the Muti Tanah) ist die Herkunft des Zinns, dem 
“eine gleiche Entstehung zugeschrieben wird. Es bedarf keiner eingehenden Ausein- 
“andersetzung, um darzuthun, dass Zinnerz durch brennendes Gras nicht reducirt 
“werden kann. Man hat auch noch niemals die geringste Spur von Zinnerz auf 
“Blores gefunden. Die uns zu Gesicht gekommenen Gegenstiinde aus Zinn hat 
“WEBER beschrieben. Sie sind siimmtlich bleihaltig.”” (Tydschr. K. Nederl. Aarde. 
Genootsch. (2) 8. 1891, p. 2830—231). It is exactly the same with P. G. Scumip- 
HAMER’s remark concerning the information of the... professors WICHMANN 
and Max Weper’, (J. c. p. 106). 


5) ]. ¢., p. 226. 


482 

mountaineers possess tin ornaments, and 3°¢ tin has little value for 
them and iron and copper is valued much higher by them. Though 
in general the correctness of these hypotheses will be readily acknow- 
ledged, we cannot help remarking that they do not prove anything, 
for in the possession of the Rokkanese objects of another nature 
are found, the origin-of whieh is as littlke known, whilst they can 
by no possibility be constructed by them. Among these are e.g. the 
lens-shaped pieces of brass, ealled by the Endehnese “mas di Rokka” 
(gold of Rokka), and the dirty-red beads known in the Timor Ar- 
chipelago by the name of Muti Tanah or Muti Salah. These are 
made of artfully manufactured glass and certainly not originating from 
the Malay Archipelago’), but of these the same story is told as of 
the tin, ie. that they appear on the surface when the grass is burnt.’) - 

With regard to the “mas di Rokka” A. feunzer indicated already 
that it is an alioy of tin and copper.*) When I was in 1888 at 
Mbawa the mountaineers asked me a gold-piece “with the leaping 
horse’ (£ 1) for it. This “gold of Rokka’ can no more be originating 
from Flores, for a nation that stands so low, is not able to manu- 
facture such an alloy.’) With respeet to the so-called tin objects the 
same can be asserted. As early as 1884 it was known, that they 
consist in reality of an alloy of tin and lead, a fact which has not 
been taken into account, in the first place C. J. vAN ScHELLE did 
not do so, not even afierwards, when a piece of “tin” obtained 
during the campaign of 1890 appeared to consist of 59,8°/, tin and 
40,2°/, lead. *®} Max Weper brought likewise into relief, that the 
bracelets bought by him in 1858 were composed of these two 
metals.") The fact communicated by him that the natives of East 


1) This subject was treated very elaborately by G. P. Rourramr (“Waar 
kwamen de raadselachtige moetisalah’s (aggrikralen) in de Timor-groep oorspron- 
kelijk vandaan ?”’ Bijdr. v. de T. L. en Vk. (6) 6. ’s Gravenhage 1899, p. 409— 
675). 

2) J. E. Teysmann. Verslag eener botanische reis van Timor... Natuurk. Tyd- 
schrift van Ned. Ind. 34. Batavia 1874, p. 350. — S. Roos. lets over Endeh. 
Tijdschr. voor Ind. T. L, en Vk. 24. 1877, p. 501. 

») Mineralogisches aus dem Ost Indischen Archipel. Tschermaks Mineralog. Mittheilg , 
Wien 1877, p. 3U6. 

') With regard to copper, it is quile certain that at least since the middle of 
the 18th century it was imported into Flores, (J. C. M. RapemaAcHER. “Korte be- 
schrijving van het eiland Celebes en de cilanden Flores, Sumbawa, Lombok en 
Bali.” Verhandel. Batav. Genootsch. vy. K. en W. 4. Batavia 1786, p. 252.) 

5) Koloniaal Verslag van 1891, p. 26. 

6) “Mededeelinger over zijne reizen in Indié.”’ Tijdsch. K. Nederl. Aardr. Gen. 
(2) 7%. 1890, p. 457. — Ethnographische Notizen tiber Flores und (elebes. Intern. 
Archiy. f. Ethnographie, Suppl. 3. Leiden 1890, p. 15, 16. 


483 


Flores opened tins in order to work the solder into bracelets ete, 
made VAN ScsELLE remark that such an idea, with regard to the 
Rokkas, “must be rejected as utterly untenable’. Weber on the con- 
trary had positively asserted that this origin of the tin objects of 
the province of Rokka was unacceptable. The fact that among the 
constituents of the bracelets in question lead occurs, the import of 
which was in former times as little known as that of tin, would 
lead to the conclusion that this metal must likewise be originating 
from Flores itself. 

Leaving out of consideration the fact that lead-ore occurs only 
sporadically *), nobody will certainly suspect the natives of under- 
standing the art of reducing the metal from it. 

A boy of fourteen years who was taken prisoner in 1890 with 
the object of being able to interrogate him, rightly remarked “he 
“could not possibly give any information concerning the tin; the tin 
“that is in their possession, they have as pusaka from their ancestors’. *) 
If one should object that objects regarded as pusaka are as a rule 
higher valued, we may point out that for several years, the gold 
that is brought by Australian horse-dealers in the shape of sovereigns 
to Sumba, from where it has found its way to Flores is more to the 
taste of the natives. During the bad harvests which are by no means 
rare, they are moreover compelled to part with objects that are 
dear to them, in order to obtain food. 

Consequently we come to the conclusion that the metallic objeets 
in the Rokka territory are not originating from the island itself, but 
that they were imported in former times. Their origin is as unknown 
as that of the different metallic objects found with the natives of 
other islands. 

The last question that must be answered is, whether the geolo- 
gical condition of the island is of such a nature, that there is any 
prospect of being able to detect tin-ore — in whatever form it 
may be. The following summary may serve for this purpose. In 
Western Flores, the eastern frontier of which is situated between 


1) Galena was found by J. J. PANNEKOEK VAN RHEDEN in small quantities in 
the neighbourhood of Lowo Sipi (Endeh) and in the penimsula of Batu Asa 
(Manggarai). J. P. FReyss supposed that the same mineral occurs near Rium and 
near Geliting on the north-coast, which is very unlikely. R. EverwisN mentioned 
lead from Mount “Himendiri in Western-Timor” (Jaarboek van het Mijnw. 1872. 
I, p. 261). The mountain is really called “Ilimandiri” and situated in Eastern 
Flores. The piece mentioned is an augite-andesite containing hematite, lead however 
is not present at all. 

2) Java-Bode, Tuesday 8 July 1890, N°. 154. 


wo 
Ww 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


484 


120°53' E. on the north- and 120°47' E. on the south-coast, an 
orographical difference presents itself already between the northern 
and the southern part. Here very accidented grounds, steep moun- 
tains 2646 m. high, and deep valleys and ravines, yonder a more 
hilly region in which only few mountains reach a height of 1000 m. 
and more. This northern part is chiefly covered by a formation, to 
which J. J. Pannekork vAN Rugpen has given the name of Reo 
formation, and which consists of limestones — especially coral lime- 
stone — resting occasionally on eruptive rocks and sometimes 
enclosing volcanic products. Here and there they are covered with 
tuffas'). PANNEKOEK writes regarding the organic remains that are 
found: “A cursory investigation stated the presence of: Orbitoids, 
“Corals, fragments of Spatangus, Natiea, Corithium, Conus, Lima (Pla- 
“ojiostoma), Ctenostreon, Gervillia, Isocardia, Teredina’. A curious 
mixture indeed. It is to be hoped that this “cursory” examination 
may soon be followed by a more correct one. From the remark 
that the strata of the isle of Rindja, “seem to be younger, most 
“likely tertiary” we must deduce that he supposes the sediments 
of the Reo formation to be of a mesozoic age, which however cannot 
be the case. H. Zor.ineer has already drawn the attention to the 
similarity of these strata with regard to their petrographic character 
with those of the south-coast of Java (Besuki, Kediri)*). They have 
entirely the character of neogenic rocks, as appears already from 
the occurrence of Globigerina limestones *). PAaNNekorK however 
rightly makes distinction between these and the younger pleistocenic 
coral limestones, as they are found in the isle of Longos in the 
neighbourhood of Reo. On the bay of Reo they rest on andesite 
conglomerate. *) A continuation of the Reo formation is most likely 
still found as far as the Kolitang Bay (Soho Kolitang) 120°77' E. 
J. F. Horpr found eastward from the exteusive plain a low range 


1) Overzicht van de geographische en geologische gegevens verkregen bij de 
Mynbouwkundig-geologische verkenning van het eiland Flores. Jaarboek van het 
Minwezen in Ned. Indié. 40. 1911. Batavia 1913. Verhandel. p. 217—218. 

®) Verslag van eene reis naar Bima en Sumbawa .. . . Verhandel. Batay. Gen. 
y. K. en W. 27. Batavia 1850, p. 14. Remarkable is his annotation accord- 
ing to which at Badjo (meant is perhaps Padja) a day’s journey behind Bari 
a hot spring is found, forming a pond, on which a brownish mass floats, which 
hardens in the air and can be used for tarring proas. 

8) J. W. Reraers describes likewise from Dangkawai 15 kilom. S. W. from 
Reo, a limestone containing foraminifera. (Jaarboek van het Mijnw. 24. 1895, 
Wet. ged., p. 135) 

4) A. WicumaNN. Bericht tiber eine .. . . Reise nach dem Indischen Archipel. 
Tijdschr. K. Nederl. Aardr. Gen. (2) 8. 1891. p. 194. 


485 


of hills consisting of limestone, and in the plain itself a few isolated 
hills of limestone °*). 

Up to the present moment only younger tertiary and post-tertiary 
eruptive rocks were found in the entire southern half of Western 
Flores. In the utmost south-western part i.e. in the Madura Bay the 
Siboga Expedition collected in 1899 rocks that on more exact examin- 
ation proved to be augite-andesite. According to D. F. van Braam 
Morris Mount Sosa 1212 m. bigh farther westward 8°46’ S, 129°58’ E. 
must be a still active voleano’). By the voleano called by him 
Toda (5000 ft.) will most likely be meant Potjo Wai L740 m. high, 
the highest mountain of the province of Todo. Potjo Leo 2696 m. 
high was already called a voleano by J. P. Freyss *) and is still 
active according to Braam Morris. J. W. MergrsurG, who marched 
along its slopes in 1890, does not remark anything in this regard *) 
Potjo Lika (2212 m.) situated in the immediate neighbourhood to 
W.N.W. is, according to PANNekork’s map, voleanic, and the same 
can most likely be said of Potjo Rea (2006 m.) and Mata Wae (2077 m.) 
rising at a short distance. J. W. Reremrs has microscopically examined 
the rocks collected in this region by J. W. Mewreure.*) He mentions 
pyroxene-andesite from the Wai Renu near Dége, quartz-augite-andesite 
of the same place, quartz-hyperstene-andesite and hornblende-hy per- 
sthene-andesite from the Wai Leédé near Rute at the N.E. foot of 
Potjo Lika, hornblende-hypersthene-andesite from the Wai Soki, 
between Lidi and Todo, pyroxene-andesite from the Wai Madjo near 
Todo, hornblende-pyroxene and hornblende-hypersthene-andesite from 
the Wai Mau, a tributary of the Mése, 9,4 kilom. N. from Nanga 
Ramo. Toren Island 780 m. high (8°54’ §., 120°15,4’ E.) °) situated 
to the south of this place is most likely also of volcanic origin. 

According to PaNNEkork’s map the whole region situated between 
Nango Ramo and the Aimeéré Bay, the frontier of Western Flores 
is of a voleanie nature. It is wellknown, that Mount Komba (926 m.) 


1) Verslag van de reis van den controleur Honpr naar de Noordkust van West« 
Flores, Tijdschr. v. Ind. T., L. en Vk. 36. Batavia. 1893, p. 292. 


2) Nota van toelichting behoorende bij het contract gesloten met het landschap 
Bima. Tijdschr. v. Ind. T. L. en Vk. 36. 1893, p. 186. 


8) Reizen in Manggarai en Lombok. Tijdschr. v. Ind. T. L. en Vk. 9. Batavia 
1860, pp. 506 —507. 

4) Dagboek van den controleur J. W. Merrsurea, gehouden gedurende zijne reis 
door het binnenland van Manggarai. Tijdschr. v. Ind. T. L. en Vk. 36. 1893, p. 290. 

5) Mikroskopisch onderzoek van gesteenten uit Nederl. Oost-Indié. Jaarboek van 
het Mijnwezen 24. Amsterdam 1895, Wet. ged., p. 135. 


6) Also called Pulu Ramo, Nusa Sigo, Gili Enta or Embuanga. 


486 


and Mount Lumu (663 m.) rising on the west-side of the mentioned 
bay over Sosi are extinct voleanoes. 

The expedition of 1890 had communicated regarding Central 
Flores that in the province of Toa, in the river-basin of the Nanga 
Koli, they had marched exclusively through a volcanic territory. In 
the upper-river-basin of this river, in the neighbourhood of Soa 


(about 8°40’ S., 121°2’ E.) — one of the repeatedly mentioned 
finding-places of tin-ore — Pannekork found at a height of = 400 m. 


a territory of horizontally stratified marls with interjacent light-yellow 
tufas containing impressions of leaves, molluscs, insects and fishes. 
He supposed these strata to be sediments, deposited in a fresh-water- 
basin and called it Soa formation '). More eastward, between Mautenda 
and Dondo on the North-coast another territory is situated whieh, 
according to PANNEKOEK’s map, is covered by sediments of the Reo 
formation. 

The southern half of Central Flores, on the contrary, contains most 
of the still active voleanoes of this island. To the East of the Aiméré 
Bay rises in the first place Inije Rije (Imé Rié) 2494 m. high, more 
known by the name of Gunung Rokka, which is in a solfatarie 
activity. Winiiam Brien saw it smoking for the first time on the 
229d of August?) and Pannekork perceived on his visit in 1910 
that the solfataras are situated on the east-side of the crater bottom *). 
The long ridge of the Langga Mountains seems to be, according to 
PANNEKORK, a Somma-edge of Mount Rokka. To the East of this 
mountain rises Watu Sipi 1466 m. and another mountain 1533 m. 
the name of which is unknown. Both are extinct volcanoes. In 
the North-east of the Rokka a group of voleanoes is found that are 
no longer active among others Kopo Lebo, Wolo Mere, about 2000 m. 
high, Pipodok, Wolo Lega, Lebi Saga, which were discovered during 
the military expedition of 1890 °). 

Inije Lika (Inié Like) 1600 m. high, hitherto entirely unknown, was 
discovered in 1910 in North Ngada and described by G. P. Rourranr °). 

1) Eenige geologische gegevens omtrent het eiland Flores. Jaarboek van het 


Mijnwezen 39. 1910. Batavia 1912. Verhdl., p. 135. — Overzicht van de geogra- 
phische en geologische gegevens.... van het eiland Flores. Ibid. 40. 1911. Batavia 


1913, p. 220—221. 

2) A Voyage to the South Sea undertaken by Gommand of His Majesty. London 
1792, p. 246. Dr. R. D. M. Verpeex kindly informs me that this is a mistake. 
Instead of Mount Rokka has to be put Mount Keo. 

3) Eenige geologische gegevens. as quoted p. 135—136. 

4) P. G. SCHMIDHAMER as quoted p. 389, 390, 393 and map. 

5) De Inije Lika op de hoogvlakte van Ngada. Tijdschr. K. Ned. Aardr. Gen. (2) 
27. 1910, p. 1233—1239, vide likewise J. J. PANNEKOEK VAN RHEDEN, Overzicht van 
de geographische en geologische gegevens. l.¢., p. 219, 223. 


487 


The heavy eruption, lasting only five hours, took place in 1905. 
About- Ambu Rombo 2147 m, high, also called Suri Laki, better 
known by the name of Gunung Keo, we do not know much more 
than that it has been for more than half a century in a situation 
of solfataric activity. According to PAnNnrKork') the solfataras are 
especially situated in the neighbourhood of the northern edge of the 
top’). As far as it is known only augite-andesite is found as 
rock on the coast. Ngaru Tangi (1537 m.) rising over the S. W. 
corner of the Endeh Bay is a voleanic ruin. 

In the territory of the Endeh Bay the western part of its north- 
coast, especially the environs of Nanga Pandan, was examined in 
1910 by Jon. Exserr*). He wrote in his first communication that 
Central Flores had been “durchquert” *) by him and that he had 
found: gray wackes, diabase-tufas, melaphyre-breccias, quarzites, marls, 
which were perhaps{ of palaeozoic age. In his work published 
two years afterwards he does not mention these at all, neither are 
the above-named rocks found back in it, but quite different ones 
are indicated. Referring to the determinations of M. BrLowsky and 
G. Rack he says, that he has found on the Wawu Manu Balu as 
fundamental rock hypersthene-diorite-porphyrite, over it hornfels, 
which was succeeded by tufa-rock. On the steep declivities of 
Woro Weka in the valley of Oto Weka he perceived at the bottom 
augite-diorite over it hornfels and further quartz-sandstone. He 
surmised the existence of a contact of the plutonic rocks‘). In 
GrorG Rack’s deseription of the collection gathered by Enprrr (39 
specimens in all) however the name of not a single one of the 
above-mentioned rocks occurs. On the contrary he describes from 
the river Manu Bala dacite and andesite, from Oto Weka and 
Langa Weka exclusively andesite!"). According to Ensert a gray 
limestone containing numerous Globigerina’s and a few Rotalia’s 
occurs near cape Ngaru Kua on the North-coast of the Endeh Bay ’). 


1) J. J. PANNEKOEK VAN RuepEN. Kenige geologische gegevens. |. c., p. 
136—137. — Overzicht van de geographische en geolog. gegevens... |. ¢., p. 220. 

®) A. Wicumann. Bericht tiber eine... Reise nach dem Indischen Archipel. 
Tijdschr. K. Nederl. Aardr. Genootsch. (2) 8. 1891, p. 231. 

8) B. Hagen. Bericht tber die von Dr. ELperr gefiihrte Sundaexpedition des 
Frankfurter Vereins fiir Geogr. und Stat. Petermanns Miltlg. 56. 1. 1910, p. 308. 

4) A somewhat eupbemistic expression, if we consider that the direct distance 
between Nanga Pandan and Geni is only about 10 km. 

USGI ZO. 

6) Petrographische Untersuchungen an Ergussgesteinen von Sumbawa und 
Flores. N. Jahrb. f. Min. Beil. Bd. 34. 1912, p. 73—82. 

ON MG (ce fon PADI 


488 


Also at Liana in the northern part of the province of Endeh PANNEKOEK 
found a lime stone rich in Foraminifera, in which moreover fragments 
of quartz, plagioclase and biotite were detected). From this it appears 
that the limestone is younger than the dacite. In the valley of 
Ndona, eastward from Ambugaga, I found a boulder of Globigerina- 
limestone. For the rest effusive rocks with their tufas and loose 
eruptive materials are prevalent in this region. The southern part 
of the peninsula of Endeh is formed by Mount Ta, usually called 
Gunung Api (6385 m.). The material from which it was formed is 
angite-andesite. For a long time it has been in a solfatarie activity. 

To the north of this mountain rises Pui or Gunung Medja only 
394 m. high, which has retained a regular craterform’). In a 
northern direction Mount Kengo (514 m.) and Mount Wongo (723 m.) 
which Ensert regards as the two cupolas of one encircling mountain, 
are connected with the peninsula of Endeh*). Most likely the 
eruption of a mountain, situated behind Brai, in 1671, which P. J. 
Vurn mentions*) relates to Kengo, and not as I supposed formerly 
to Pui. 

To the West of the Ndona valley rise Geli Bara (1731 m.) and 
Geli Mutu (1494 m.), the latter of which is in a situation of solfatarie 
activity °). The pyroxene- and labrador-andesites originating from this 
territory were described by G. Rack’). I found in 1888 in the 
valley of Ndona numerous boulders of dacite, labrador-andesite, 
augite-andesite and on the deelivity of the mountain andesite. To 
the east of volcano Ndona Expert still mentions Nduri, which has 
a solfatara’). The island of Nusa Endeh situated in the Endeh Bay 
is likewise of a volcanic origin. 

In the eastern part of the island of Flores the limestone formations 
have become very scarce. The little information we have about it 
is limited to the hillrange in the W.N.W. of Sikka situated in the 
province of Liu on which, according to H. Ten Karr, the villages 
of Kiara (+ 275 m.),and Riipuang (+ 350 m.) are situated.*’) The 
rock collected by him is a Globigerina limestone. In the farthest 


1) Overzicht van de geogr. en geolog. gegevens |. c¢., p. 219. 

2) A. WIcHMANN l.c., p. 222. 

8) l.c., p. 202. 

*) Het eiland Flores. Tijdschr. voor Nederl.-Indié. 1855. Il. p. 157. 

®») J. J. PANNEKOEK vaN Ruepen. Eenige geolog. gegevens l.c., p. 157. — 
J. Expert. Die Sunda-Expedition. II. 1912, p. 202. 

6) l.c., p. 78—82. 

D) lacsmpsecO2: 

*) Verslag eener reis in de Timorgroep en Polynesié. Tijdschr. K. Nederl. Aardr., 
Gen. (2) 11. 1894, p. 221, 


489 


Northeast occurs then limestone in the vicinity of Tanjung Bunga 
or Kopondai, the well-known Cape Flores, to which the island owes 
its name. At a distance of 300 m. eastward from the cape men- 
tioned, G. A. J. VAN DER SANDE discovered a grotto with stalactites. 
And at last, according to A.J. lL. Couvrnur, coral limestone is found 
to the North of Larantuka from Panté Lela to Panté Beli Beting, 
especially between the village of Labao and Ili Labao. 

The entire remaining part is covered with volcanic material the 
monotonousness of which is only interrupted by the numerous partly 
still active voleanoes. In the North westward from Maumeri rises 
the voleanic ruin of Kiman Buleng (1446 m.). Gunung Dobo or 
Iliang (900 m.) situated behind Geliting but nearer to the South- 
coast is on the contrary still active. 

Most known, though likewise not sufficiently examined, are the 
voleanoes situated on the East-coast of Flores. For times immemorial 
Ilimandiri (1570 m.) has not given any sign of activity. The rock 
of which it is composed is chiefly augite-andesite.*) Kabalelo (1075 m.) 
situated eastward is an old voleanic ruin. *) Westward from it Leworoh 
is situated where on the 16% of March 1881 an explosion-crater 
formed itself.*) The largest, highest and most active voleano however 
in this territory is Lobetobi, consisting of two cones Lakilaki 2170 m. 
high and Parampuan 2263 m. high. 

G. EF. Typrman perceived about 37 km. westward from Lobetobi 
a high voleanie cone; most likely Dara Woér is meant by it. *) 

As appears from the above, there is in Flores no room for 
praetertiary sediments and eruptive rocks. Repeatedly however the 
existence of such like rocks in the form of boulders was hinted at. 
Near the bay of Bari I found in 1888 quartz-porphyry, clay slate 
and quartzite.°) I may now add to this the communication that in 
the river Reo amphibole-granite and diabase occurs, the hornblende 
of which has changed into chlorite. More eastward in the territory 


1) Ken dicnstreis benoorden Larantoeka (Oost-Flores). Tydschr. K. Ned. Aardr. 
Genootsch. (2) 25. 1908, p. 554. 

2) A. |WicHMANN I. c., p. 159. — G. Rack. Beitriige zur Petrographie von 
Flores. Ceutralbl. f. Mineral, 1913, p.p. 134—139. — H. Méutu described from 
Okka, situated on the south-western extremity of Ilimandiri sanidine-trachite and 
Hauyn-andesite (N. Jahrb. f. Min. 1874, p.p. 694—697). The determination however 
was not correct. 

3) J. P. vAN DER Stok. Uitbarstingen van vulkanen... gedurende het jaar 1881, 
Nat. Tidsch. Ned.-Ind. 42. 1882, p. 241. 

4) Hydrographic Results of the Siboga Expedition, Siboga Expedition 3. Leiden 
1903, p. 56. 

lca oo. 


490 


of the mouth of the Nanga Koli A. F. H. Heuscn collected in 1890 
according to PANNEKOERK ') quartzite and greywakke(?). On the south- 
coast at Nanga Mbawa I found granite (read quartz-diorite) and 
gabbro*) and finally in the valley of the river Ndona quartz-diorite. 
None of these rocks were ever found as rock, they are con- 
sequently at least “auf tertidrer Lagerstatte’. They are the last 
remains of rockmasses that got into the conglomerates by washing 
from which they got afterwards free again. 

The oldest formations of Flores belong to the effusive rocks of 
the character of dacites, labrador-andesites and hornblende-andesites 
with their tufas, on which those of the limestones of the Reo-form- 
ation and those of the tuffas of the Soa formation follow. They 
were uncovered by subsequent elevation. Afterwards the island was 
over its entire length the scene of violent voleanic eruptions, from 
which the only partly known crater mountains proceeded. The 


material produced by them consists — as far as our knowledge 
reaches — exclusively of pyroxene-andesites belonging to the Pacific 


type of rocks. The younger coral limestones occurring only spora- 
dically have only been formed after the formation of the volcanoes. 

Von Scuenie’s postulation that the bottom “to the north of Mount 
Rokka is very rich in tin-ore” appears to have been not only vain 
but also very expensive. 


Mathematics. — “The theory of the combination of observations 
and the determination of the precision, illustrated by means of 
vectors.’ By Dr. M. J. van Uven. (Communicated by Prof. W. 


” 
’ 


IC APTEYN) 
(@ommunicated in the meeting of June 27, 1914). 


By L. von Scurutka*) and C. Ropricuez*) a method has been given 
of illustrating geometrically the theory of the combination of obser- 
vations by the method of least squares, namely by means of vector 
operations. RoprieurZ however chooses in the case of rigorous equations 

idition another way, whilst VON ScHRUTKA, who consistently 


1) Overzicht der geographische en geologische gegevens I. c. p. 229. 

*) I. ce p. 229. 

3) L. von ScHruTKA, Eine vektoranalytische Interpretation der Formeln der 
Ausgleichungsrechnung nach der Methode der klemsten Quadrate. Archiv der 
Mathematik und Physik. 3, Reihe, Bd. 21, (1913), p. 293. 

4) C. Ropriauez, La compensacion de los Errores desde al punto de visto geo- 
metrico. Mexico, Soc. Cient. “Antonio Alzate’’, vol. 33 (1913—1914), p. 57. 


491 


operates with vectors, restricts himself to two variables and one 
rigorous equation of condition. 

It is our purpose not only to extend their method to the case of 
an arbitrary number (JV) of variables and an equally arbitrary 
number (») of conditions, but also to derive the wezght of the unknown 
quantities in the same way. 

I. There are given N quantities wv, 7, 2,... which are to be deter- 
mined from (approximate) equations of condition (equations of 
observation) : 

qe+tbhy +qze+...+m=0 Te epee On 

These equations have the weights g; resp., and so are equivalent 
to the equations 

aVg-t + bY g-y + aVg.2 +... +mVg=0 C= oss 
each of which has the weight unity. 

We now introduce 

ah aV 9 pee bY gi fe V9 me mi V Gi f 
Tea es ey ie 
A— miles], B= V [bz C= 2V [gras [gimi*] 
AAG: —=0,|-gi0a . By BUA gue, Ci C0 Yi; (/G;. 2 0: 


ay 


el Mi oi. 
[| | denoting summation over 7 from 1 to n. 
So the equations of observation run in the form 
A;+ B+ ¢C;+...M=0 il Ieee) 

We now consider A;, B;, C;,... 4; as the components of the 
vectors WU, 3, €,..©, resolved parallel to the rectangular coordinate 
axes of an n-dimensional space. Thus the tensors are 4, B,C... J/, 
@;, (Fi, Y¥i,++- ui representing the direction cosines. 

The set of m equations of observation may now be condensed in 
the single vector-equation 

YL SLC +...4m—0, 

which expresses, that the vectors 2, %,€,...9¢ must form a closed 
polygon. The coefticients a;, ;,¢;,... and the weights g; being given, 
the unit vectors a,6,c,... of the vectors U,%,&,... are determi- 
nate. So the vector-equation requires that 2% may be resolved in the 
N directions a,6,¢,..., in other words: that lies in the V-dimen- 
sional space Ry, determined by the vectors a,6,¢,... and called 
the space of the variables (or unknown quantities). 

In consequence of the errors of observation this condition is not ful- 
filled. The most probable corrected value of M is the projection of 
® on the space Ry of the variables. 


492 


Denoting the projecting vector by 8 (tensor A, direction cosines 
x;, components A;) we have really 
U+B+E C+... FM=HK. 
As & is perpendicular to U, 3, 6,..., we have 
Q,k)=0, (8, K=O, C6 R=, ete 
or 
GLa => (o: 2 10; ly7iAG] =, ete: 
or because 
R=A4+ B+ C4...4+ M4=qG4A4+ 8:8 +7C04+...4+ mM, 
[a7] A+ [afi] B+ faiyi]C+...4+ [a Mi] =0, 
[Pia] A+ [@?7] B-+ [Fix] C+...+ [FM] =, 
ya] At [yi fi] B+ [yi?] C+...+ [yd] =0, 


By multiplying these equations by V[giai?], V[gibi?|, V[ gic’), 
. resp., We obtain the ‘normal equations” : 
[gia] @ + [ocai bi] y + [gcaicz] s+... + [giaim:] = 0, 
[gbiaila + [oib?*)])y + [gibi] 2 +... + [oibimi] = 0, 
[giccai]a + [gcbily -+ [gie?]e +...+ [gicim:] =9, 


II. After these developments which also are given by VON ScHRUTKA 
and Ropricurz we proceed to determine the weights of the variables. 

For this we notice that all the quantities J/; have the weight 1, 
and therefore have an equal mean error ¢. From this ensues, that 
the projection of 2X in any direction has the same mean error é. 

We have to investigate the influence on % due to the variation 
of M, if the other variables B,€,... do not undergo that influence. 

A variation of % which does not displace the foot on Ay of the 
projecting vector &, does not act upon any vector 4, 3, ©... So we 
have only to do with a variation of the projection ®’ of Mon Ry. 
In order to leave the vectors 3, &,... intact, the foot is to be moved 
in a direction $§ perpendicular to 3, &,..., and, because it lies in 
Ry, also perpendicular to 8. 

Denoting by 6; the direction cosines of 8, we may put the equation 

(4, 8) + (Mm, 8) = 0, 
obtained by multiplying the equation of observation scalarly with 
8, in the form 
A [ajo; |] = — MU, 

M, designating the projection of MN on 8. 

As M, has the mean error ¢, the mean error ¢4 of A equals 


493 


é 


é4 = = 
[ao;|? 


whence 
GA = la70; \7- 

The vector 8, lying in Ry, may be resolved in the directions 
a,%,¢,... Denoting its components in these directions by X,Y, Z,... 
we find 

B= Xo Picea cee 
or 
6;= Xa;+- VP; 7; -+ -.-. 
Now, 8 being perpendicular to &, €,..., whence | /?; 6; |=0,| y; 6; |=0,.., 
we have ‘ 
— [o;? == xX [ai 6; | 
or 
1 


X = ——_.. 
[a; 6; 
From the equations 


[az03|(—= (256; — 05) (7:6; |= 078: 


xX 5] 
which may also be written 


[a*] X + [afi] Y + [aiyi] 7+ -..= 


[(Piei] X + [82] Y + [ivi] 7+ --= 
[ye:i]X + fifi] Y + 7) 2+--= 


or 
-[ai?] X? + [a; i] XY + [eiyi] XZ + .. —1=—0, 
[Pia;] X? + [7] XY + [Aixi] XZ + 
[vi aj] X? + [vi (7: | XY+ [yi] A Z+.t0=0, 


the first unknown quantity X? takes the value 
oes ae, 
[a o;]? = GA 
The reciprocal value of the weight of A is therefore found to be 
the first unknown of the “modified normal equations”. 
Putting further 
X=EY[gia7], Y=Hyv[gib7], 2Z=—SV [gic], --- 
the modified normal equations pass into 
[giai?] §* + [giaibi] Sy + [giaics]§5+..—1=—0, 
[gi b; a; | 5? + [gi bf] Sy + [gi bic) 65+..+0=0, 
[gicra: |] §? + [giccdi] y+ [gie?] 66+ ..+90=—90, 


494 


Now, from A=xV|g;a;7] ensues 
€4= &/ [gia], 
hence 
een eee eat ig es Ca | 
les is [qia;? | Si [gi ai” | ee 
which is the well-known theorem on the weights of the variables. 
Example: 3 equations of observation with 2 variables. 


M The unit-vectors a and 6 determine a 
plan &,. The extremity J/ of —M=OM 
mM is projected on this plane in the point 
A M’. OM’ is resolved parallel to a and 6 
: .y into the components OA=% and OB=%, 
In the plane A, (4,3) the vector 8 is 
M aS "erected perpendicular to 3. On this vector 
A A OM—=-—M® and OA=Y have the same 
Fig. i. projection OA,—= M,. This segment J/, 
has the mean error €; the variable A, i.e. the segment OA there- 
; € 
fore has the mean error &4 = PETE 


III. We now suppose that besides the n approaimate equations 
of condition (equations of observation) » rigorous equations of con- 
dition are given, viz.: 

An pie + bn+ jy Sip Gaeta oo ge Og =D (RM con D) 

For the sake of regularity in the notation, we will also provide 
these equations with factors g,4; (which afterwards disappear from 
the calculation). Thus we really operate with 


Ant jV Int j-% + ont GV In45-Y Font gV Int y-2 feet Wnt 5 V Jn+j—0(J=1)-0)- 
Agreeing, that eal now means a summation over 7 from 1 to 
n+», we may, retaining the notation used above, consider 2, 3, 
@,..., M as vectors in a space of m+ v dimensions. 
The vector-equation 
YB ie 22 Wt 0 
is again not fulfilled on account of the errors of observation. The 
last r component-equations (2 + 1)...(-+ ») however hold exactly 
this time. 
Putting again 
Y4+HLC+. .+mRM=—K 
the » projections An4i,.. Any, of # must be zero, whence 
tn4+; = 0 (j= 1,..>). 


495 


So the vector ® is perpendicular to the space R, ‘of condition” 
determined by the coordinate-axes 7,4; and therefore cannot generally 
be any longer assumed to be perpendicular to the space Ry (2, 3,6...) 
of the variables. # lies in the n-dimensional space Pn ap4j= M4; 
(j=1,.v), which is parallel to the space R, “of observation” determined 
by the axes a, (h=1, .. 7). 

The parallel-space f', cuts the space Ry of the variables in a 
linear space of NV + 2—(n-+-r) = N—»y dimensions, which we shall 
denote by e'y_,. This latter is parallel to the space @y_, of inter- 
section of the space /, of observation with the space Ry. 

We now project the extremity of M lying in R', in this space 
on the space e'y_, of intersection. The projecting vector will now 
be the ‘correction-vector” §. 

Translating & to the origin into the vector OP, OP wiil be per- 
pendicular to the space gy—, common to Ry and R,. 

Next we construct the normal space of @y—, which passes through 
the origin O. This space has n—-- vy —(N—v)=n-+ 2r»—WN dimens- 
ions. It contains the space &, of condition (as normal space of &,), 
further the line OP, and also the normal space of n+ »— N 
dimensions which can be drawn from P perpendicular to Ry. 
This latter space therefore lies together with #&, in a space of 
n-+2r— N dimensions and thus cuts #, in a space of (n-+r—N) + 
+ » — (n+2r—N) =O dimensions, consequently in a point. As for 
this point Q, it thus lies both in A, and in the normal space drawn 
from P perpendicular to Ay, from which among other things 
follows, that PQ makes right angles with each line of Ry, more 
particularly with the vectors W,%,@,... So, projecting OP and OQ 
on 4, these projections are equal. The same holds for the projections 
un 2), Crook 

Representing OQ by the vector St'(K', x;', K;'), we have, as St 
lies in R, 


Ky! = 0 and x;' = 0. (A=1,...n) 
From 
Get) (I) (St) i ( Da (ts i — (RO), 
follows 
EG [oe nee Nl = RG [estrella see (sil KG [ote Sigil 2 [see |i Ee [ee Vg] 5 «2 
AS: tpi Oh tory sa. the sum [x;e;| is only to be ex- 


2 


tended from 1 to n; hence [x;@; |] = S x,¢, = [*naq}'; and since 
1 


z, =0 for h=1,..n, the sum [x,'@;]| is to be extended from n--1 


496 
v 
to n+», so that [x;'a; | Sh On — [%n4j'en4j |" Here and in 
1 


7! 


what follows [;|' will denote a sum over h from 1 to n, and [n4; |" 
a sum over 7 from 1 to ». 
We may therefore write 
[e@,Ky)' = [an+; K45]", 
or, because 
Ki — Ae Be Oe ae ee yiC +... + Mi, 
[en?)'A + [enPi]'B +- Leaya]'C + .. + [andG]' = [en4jKn4j]"s 
[Pren}'A + [Fr B + ([Pryi]'C + + (PM! = [2n4j Kn, 
[ynceal'A + [vaFil'B+ [yO + + [vaMi]! = [vn jKn4j7': 
Putting 
Cn jpg Pn j=PP's Prt j= Ty's + Kny'=— Qi Mn4j—=MG, mn j= mj), 
we have 
fan?) A = enh Be lanyniGeonen [en Ma] fe [a;'Q;]" == (I) 
[PrenJA + [2VVB + [Prvi]'C + -. + [PaMal + [7;'Q;]"=0, 
Lyneny'A + [ynPalB+ [yO +... + LyaMal' + [77 Q)"=09, 
Introducing 
aj V [gi a?) PV [9 627] 
S77 a ae = er a 
V Inj , V oni 
i'V [oie] 
V Int) 
we obtain, after multiplying successively by Vigia;*], V(gib.7), 
Vigier), = 
Lonan?)'@ +- Lonanba]'y + [onanen]'e + -- + Cgnanmal! + [ay'g;]" = 0, 
Lonbranl'e + Landa? ly + Lonbrenl’e +--+ [gabama]' + [b;'q;]" = 0, 
Lonenan)'e + Loneabay'y + L[gncn*}'2 ++. + [gncnmal' + [e;'q/]" = 0, 


’ 


Qj = On 5 = 


Ul 
Cj = 4 yj = 


19 9 = QV Ont; 


N equations, which together with the » conditions 

aja + by + c'z2+.. + mj =0 
serve to determine the N variables «, y,2z,... and the » auxiliary 
quantities g;. 


IV. In order to determine the weights of z,y,z,..., i.e. of 
A, B,C,..., we must examine the influence undergone by % from 
a variation of MN, the vectors 3, &,.. remaining unaltered. 

A variation of ® only acts upon %, 3, €,.. when the foot of & on 
the space 9'y_, of intersection moves. If the foot is fixed, #* may freely 


49 


~) 


move in the space S, common to the normal space of @!y_, (of n+ 2» 
—N dimensions) and the space 7’; parallel to 2. The space S obviously 
has (n--2r—N ) + n —(n-+v) =n + v— N dimensions. A component 
of M in this space has no effect on the vectors U%, 3, ,... A com- 
ponent of M® will only have any effect on 2, B,&,..., when it lies 
in the normal space S’w of SS, which has n + »— (n4+-r—N)= N 
dimensions. By translating this normal space S'y to O, it contains 
both R, and oy_, (intersection of Ry and R,). 

The variation of ® will exclusively influence %, when the com- 
ponent of M undergoing this variation is perpendicular to B,€,... 

These considerations lead to the result that we want that direction 
8, which lies in S’y and is perpendicular to %,@,... The vectors 
¥, ©... determine together a space of N—-1 dimensions. The vector 
8 must lie in the normal space (of mn -- »— N+ 1 dimensions) of 
the space (8, &,...). This normal space cuts S’y in a space of 
(n+ v— N+ 1)+ N—(n+ vr) =—1 dimension, hence ina straight 
line. So there is always one and only one line 8 fulfilling the 


imposed conditions. 
Since 8 lies in S’y, i.e. in the space joining R, with oy_., the 
projection t of 8 on 2, will fall into ev_,. 
Now we have for the direction cosines 1; of the projection f of 
gon R,: 
On 


h= Sere aae 

V [on] 

As t, being a line of ey_,, also lies in the space Ay and therefore 
may be resolved in the directions %, %, &,..., we have 


(SS he OME (paar) 


ty, = Po, + Q2, + Ryn +. (= 1,---n) 
ie QP Ryn 0. (7 = 1,..0) 
Putting 


PVG OY fora) 0 *s, = Ay for-|- = hi. .<. 
we obtain : 
wP' + fQ+yR +... =i (ie, an) 
nt jP! + Pn4jQ + yn Rh +... = 0, Gi lb) 
and, 8 being perpendicular to %, &...., 
27Ga| == 0%, Ree]| == enc (ops) Stk 
In this way we have collected n +» + N equations to determine 
the n+» unknown quantities o, and the NV unknown quantities 
Eko OE i pers Ve 
S’y being perpendicular to &, $ is also perpendicular to ®. By 
multiplying the equation 


498 


Y1 $416 +4..4M=—=K 
sealarly by 8, it reduces to 
(a, 8) + (M, 8) =0 
or 
A [ajo;] = — 

In order to determine the mean error of J/,, we remark that of 
all the lines through O in Ry t is that which makes the smallest 
angle with 8. The error of J/, therefore depends for the most part 
on the error in the components JZ, of M in the direction t. We 
may consequently write 


m. e. of M, =m. e. of Mi X cos (8, t) = € cos (8, f) 


or 
zs ae : 
€, =e [oi] =e | on. —— | = ev [o,']', 
ean) | : se | V [077] 
hence 
&s V [o,7]' 
= = 
[aioi] [aio;] 
Since 
Ls Oh aq ; 
M, =; lo;r:) = [AG xa. lor] = Ei sta | -V [on?]' = [Dfion]', 
V [on 
we have 
AYE m6, t 
7 _ She . My, 
| ioi| [ aio; | 
or, putting 
Oh 
——- = Dh, 
[ aio; | Le: 
A=— [paMil. 
1 4° [ on? | : 
Ss ety 
OA & [ajoi]? 
Introducing 
f' (Qh PI Ontj 
Xa eS BS Se ee 
[aio] [aioi] ail Baty [aves] ” ) 


we arrive at 
aX | PY 3 yiZ es. = Ph (AS i1,...0) 
@tn = ;X + Pn+j¥ + yntjZ+--=0 (ji 15 =-P) 
lapl=1 , (Cal=0 .\ irpl— 0. 
From these 2 -—+ » + V equations we ean solve the 2+» unknown 
quantities p; @—=1...2-+ yr) and the NV auxiliary quantities X, Y,Z.... 


Il 
The quantity —-—J|p,°}' in question is also found as follows 
GA 


499 


1 ‘ . ; 
= =p?) =[pilenX+(21V +724...) =X [preeny+¥ [pr Pn\+Z[piyil'+-- 


" 


= X— NX [pnp jang yl" — VY (pot yiFr45)" — Z [patra]! 
= X— [png lang jg X + Bn V + ny Z +o)! 


=X 
Returning to the original variables x,y,2,..., we derive from 
A 
Ss —— 
Vigia*] 
tirstly 
&A4 
& = ——— 
V [aai"| 
and 
ee Vall 
qa eee loner |e 
Further, putting 
V laa; | Vi[gai*] 
Li ky Saas oe Pr+j = Ken-tj Se 
Von V Inj 


X= § iovas* |; Ye) [loons ZAG Chall stelle = 


the n +--+ NV equations pass into 


L F ky 
age ibpap S cyS 2... = =, (6 == Ne oe nia) = 
ah 
Ont76 + Open tentgs +... = 01, Gly een) 
fark] = 1, [br k; | = 0, [feathered == O ener, 


whence 


Example: 2 equations of observation with 2 variables and 1 
condition. The unit-vectors a and 6 determine a plane /?,(NV=2), 
the plane of the variables. This plane euts the plane of observation 
R,(m=2) in the line ev, N--»=1), which thus coincides with 
the line t. The line OP is drawn in the plane &, perpendicular to 
on, (0. Through the extremity J/ of the vector M a line is drawn 
parallel to OP; this line euts the plane Ry of the variables in 17’. 
The veetor JIM’ —//— PO is the correction-vector 8. OJ’ is resolved 
in the directions a and 6 into the components OA = %and OL=, 
The lengths of these lines represent the most probable values of the 
variables A and ZL. 

The line PQ is perpendicular to the plane ty and meets the 
normal /, (line of condition), erected in O on /2,, in the point Q, 
The vector OQ is ealled St’. 


99 
vv 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


Fig. 2. 
erected in O perpendicular to ¥, interseets S'y in the line 8, which 
therefore is perpendicular to 3 and S&. So A and J/ are projected 
on § in the same point Ag. 

The normal plane A As VW of g cuts t in a point 7. the distance 
of which to QO amounts to J/, (with mean error ¢). The mean error 
e, of A, thus has the value &; = «cos (8,t), and that of A the value 

Es cos (8, t) 
a cas (8,0) i: cos (8,a) 


V. The errors (residuals) of M,, M,,.. Mf, are K,, K,,.. Ky resp. 
The sum of their squares is [Aj?| = A®. 

For the ease that no equations of condition are given, ® must be 
perpendicular to /y. So S& may dispose of a space of »—NV dimen- 
sions (the normal space of /?y). Hence ® has 2—N components, 
all with the same mean value ¢. Consequently 


K? = (n—N) X & 
hence 
[Ai] 
S== -——., 
n—N 
In case p conditions are imposed, & may dispose of the space S 
of n+xr— N dimensions. Consequently ® now has n+ »— NV 


components, all with a mean value ¢. In this case we have therefore 


cee L LGA 
ae n+ v—N- 


501 


Physics. — “On the measurement of very low temperatures. XXIV. 
The hydrogen and helium thermometers of constant volume, 
down to the freezing-point of hydrogen compared with each 
other, and with the platinum-resistance thermometer. By Prof. 
H. KAmMertinGH Onnes and G. Horst. Communication N°. 1444 
from the Physical Laboratory at Leiden. 


(Communicated in the meeting of May 30, 1914). 


§ 1. Introduction. The measurements which this paper deals 
with bring the investigations undertaken in Leiden for the purpose 
of establishing the seale of the absolute temperatures as far down 
as the freezing point of hydrogen, to a conclusion, in so far that a 
direct comparison has now been made between the helium and 
hydrogen scales, by measurements with a differential thermometer, 
which had the object to test the corrections to the absolute seale of 
temperatures below 0° C., obtained separately for the helium seale 
(in XIX of this series) and the hydrogen seale (partially given in 
XVIII of this series ')). For the place which the mutual control of 
these corrections occupies in the more general investigation of the 
measurement of low temperatures which is being carried out in 
Leiden, we refer to § 6 Suppl. N°. 34a. The test could be extended 
as far as the freezing point of hydrogen, after the compressibility 
of hydrogen vapour had been determined by KAmERLINGH ONNEs and 
pe Haas, Comm. N°. 127¢c. June 1912) *). Our comparison of the 
helium seale with the hydrogen seale*) by means of the differential 
thermometer to which was added a new calibration of the Leiden 
standard platinum thermometer /7¢;' (formerly Pt,) shows that a 
very satisfactory agreement has been attained in the temperature 
determinations. 


1) Compare also H. KaAMeRLINGH OnNes, CG. Braak and J, Guay, Comm. 
N°, 101@. (Nov. 1907) § 1 under 40. { 

*) In this Comm. a difference was discussed which existed between the tempe- 
rature delermination with a hydrogen thermometer according to the resistance 
thermometer Ply',-which was calibrated by means of it and the temperature deter- 
mination by extrapolation of the isotherms. According to caleulations by Dr. 
Kersom, suggested by SACKuR’s interesting‘ investigation, this deviation might be 
connected with the theory of quanta (Gomp. Suppl. N°. 30 and N® 34a § 11). 

3) The comparison of the hydrogen and helium thermometers by Travers, 
Senver and Jaquerop, Phil. Trans. A 200 (1903), p. 105, has been discussed 
in Gomm. N° 102, In general their results are in good agreement with our 
measurements, 


3o* 


S02 


§ 2. Apparatus. Two identical thermometers of Jena glass GUL, 
such as had been formerly used by H. Kammrirmcn Onnes and C. 
3RAAK, Were connected to one manometer. The arrangement was 
otherwise exactly the same as that used before. The standardmeter 
was divided into '/, m.m. and allowed a direct estimation of '/;, m.m. 
This gave a considerable saving of time, as it made the use of the 
measuring eye-piece of the cathetometer unnecessary. The amount 
of gas in the capillary was measured by an auxiliary capillary of 
much larger section, as described by Crapputs. 

Besides the two thermometer bulbs, the cryostat contained the 
platinum resistance thermometer /’;) and a large pump, which 
provided for a good circulation of the liquid. 

The hydrogen and the helium were purified by distillation, and 
were both free from other gases. 


§ 3. Calculations. The temperature for each of the thermometers 
forming the differential thermometer was calculated from the formula 
given in Comm. N°. 95e, but with a few alterations. The expansion 
of the glass f(t) of the bulb was not calculated from the quadratic 
formula given there, but taken from a graphic representation in 
whieh the curve was drawn through the points experimentally deter- 
mined and extrapolated by means of the expansion for a different 
kind of glass as determined by Cu. Linpemann. The influence of the 
different temperature function for the expansion of the glass is 
about ?/,,,° at hydrogen temperatures, at all other temperatures it 
is negligible. Moreover the volume was divided into three parts. 
a. The bulb at the temperature ¢ of the bath. >. The capillary in 
which the mean density of the gas was determined, by means of 
the auxiliary capillary: the mean density is proportional to ss he 

L 
being the pressure in the auxiliary capillary at 0°, 4 the measured 
pressure. c. The steel capillary and the volume about the point, the 
temperature of which is the same as that of the room. 

If we divide all the members of the above mentioned equation 
by the volume of the bulb it becomes 


IT i 3 Wear h, ue dvo 273 
—_ |: tO hg tga Oo ayer ae a= 
h + ath 


l+at 
273 
1+ at). : 


The provisional temperature, which is needed for the calculation 


of the various corrections, was calculated from the resistance of Pt’. 


508 


i, ; 
Even move this temperature with sufficient accuracy. The zero- 
0 


pressure for the hydrogen thermometer was H/4, = 1191 m.m.'), for 
the helium thermometer //, = 1124 m.m. Circumstances unnecessary 
to be mentioned here, had prevented these pressures from being made 
more equal. A new set of determinations in which this will be 
attended to is planned. The pressure coefficient of hydrogen at the 
above mentioned pressure was taken at 0.0036625 ; for helium at 
0.00386614, the value derived by KaAmertincH Onnes *) from the 
isothermals at O° C. and 100° C. If we ecaleulate with the pressure 
coefficient 0.0036617 deduced from the isothermals of 20° C. and 100°C, 
we find, after the introduction of the necessary corrections, almost 
the same temperature on the absolute scale. 


§ 4. Arrangement for the resistance measurement. In order to 
measure and to compare resistance thermometers two identical differ- 
ential galvanometer circuits were fitted up according to KoHLRauscn’s 
method. Both galvanometers can be read from one place, so that 
nearly simultaneous measurements can be made. This removes all 
irregularity in the temperature of the bath in the comparison of 
resistance thermometers. Two moving coil differential galvanometers 
from Hartmann and Bracn were used. With an additional resistance 
of + 1000 2 in each of the coils these are practically aperiodic in 
the measurement of resistances less than 180 2, as with all our 


other thermometers. The sensitivity is sufficient to measure ——-— 2 
100000 


with a current of + 5 milliamperes, while the condition of propor- 
tionality between deflection and current-strength is very well fulfilled. 

Test-measurements have shown, that with this arrangement resist- 
ances of about 100 2, such as our thermometers have at ordinary 


1 
temperature, can be compared to TGuGE without any difficulty. Our 


1) At these pressures even at the melting point of hydrogen no attent.on need 
be paid to the thermo-molecular pressure according to KNUDsreN (Comp. Suppl. 
NY, 34 § 7 and a Comm. by H. KamertinGH OnneEs and 8. WEBER which is 
shortly to be expected, on the determination of the temperatures which can be 
obtained with liquid helium). 

2) H. Kamertincu Onnes. Comm. No. 1020. The value is here increased by O0.0000001, 
in consideration of the value 273.09 since assumed for Too ¢, Gomp. H. Kamertinex 
Oyves und W. HL. Keesom. Die Zustandsgleichung. Math.Enz. V 10, Suppl. No, 23) 
Einheilen c, and § 820. 


504 


experience with moving coil differential galvanometers, for this purpose 
at any rate is very favourable '). 

In the manner described we attained a much greater rapidity of 
measurement than was possible by the method described in the 
previous papers of this series, and this in its turn increases the accuracy. 

We must also refer to our experience with thermometers in which 
the wire was sealed to the glass (Comm. N°. 95) § 1). For tempe- 
ratures above that of liquid air they are not unsuitable, although 
even here they are less constant than those with a free thread. 
After immersion in liquid hydrogen their resistance was found to 
have increased by about one tenth of an Ohm. Each further immers- 
ion in hydrogen carried with it a permanent change of resistance, 
so that we replaced these thermometers by other ones with free 
threads wound on porcelain tubes with a double screw thread baked 
in. After a thermal treatment, consisting in several immersions in 
liquid hydrogen followed by moderate heating, these became satis- 
factorily constant. 


§ 5. Results. In the following table the results of our researches 
are found. The two first columns contain the hydrogen and helium 
temperatures calculated from the formula given above. Column 3 
and + contain the corrected temperatures on the absolute scale 
deduced from the hydrogen and from the helium thermometer, 
column 5 contains the resistance of the platinum thermometer P¢/. 

The agreement is on the whole very satisfactory. 

We have already mentioned that with thermometers of the kind 
described an accuracy of about */,,° might be expected. Our meas- 
urements show this to be the case; only in a few points larger 
deviations occur. These can readily be explained by a small defect 
which will be avoided when we repeat the experiments, namely that 
the eryostat which had to be used was not quite symmetrically 
built. When both auxiliary capillaries worked properly this was 
not of much consequence. But (except fortunately in the determina- 
tions most important for us viz. at the hydrogen-temperatures) the 
helium capillary got out of order, so that the distribution of the 
temperature of the stem of the helium thermometer had to be deduced 
from the observations with the hydrogen capillary. This cireumstance 
has the greatest influence at temperatures at which the methyl 
chloride and the oxygen evaporated under reduced pressure, and it 
is exactly there that the greatest deviations occur. 


1) Compare JarGer, Zeitschr. f. Instrumentenkunde 1904. 


or 
S 
or 


TABLE I. 

fee | fete sO ee 9 tHe W pyr 

0 | | 135.450 
fal eesrea: |); = 23.96) |) = 23706 = 23, 94 | 122.613 | 
2 43.09 | 43.07 3.00 | 4g.07 | 112.278 
3 qps0. | 61.40 | 61.50 61.49 | 102.280 
4 79.57 79.51 79.57 79.51 | 92.422 | 
5 102.72 102.69 102.70 102.69 | 79.674 | 
6 113.58 | 113.55 113.56 113.55 | 73.629 | 
7 | 130.46 | 130.41 130.43 130.41 64.189 
8 | 182.88 | 182.81 182.82 182.79 34.180 | 
9 | 186.79 186.70 136.73 186.68 | 31.904 
10 | 195.24 | 195.15 195.18 195.13 26.988 
11 | 204.79 | 204.69 204.71 | 204.67 | 21.491 
12 212.61 212.52 212.52 | 212.50 | 17.097 
13 | 216.25 | 216.15 216.16 | 216.13 15.119 
14 | 252.80 | 252.68 252.66 | 252.64 | 1.924 
15 | 256.23 | 256.10 256.08 256.06 | 1.601 
16 | 258.56 | 258.41 258.39 258.37 1.453 
17 252.80 | 252.66 1.925 
1S 253.78 253.64 | 1.819 
19 255.20 | 255.05 1.685 
20 257.22 257.05 1.531 


The readings of P/ allow a comparison with the measurements 
of 1906—1907. 


WW 
In fig. 1 the deviations from the linear formula ¢/—= — 248 + 245 ae 


0 
are represented for all three calibrations, at temperatures above 
—-217°C. The circles refer to the calibration of 19138, the triangles 
to 1907 and the squares to 1906. For the calculation of temperatures 
in this field the above formula with the deviation curve belonging 
to it has been recently used in the Leiden researches, 


506 


2s 


Riess 

The differences between the calibrations of 1913 and 1907 are 
less than */,,‘¢ of a degree throughout. The fact that the differences 
with the first calibration (4906) are more considerable must un- 
doubtedly be attributed to the mechanical treatment of the wire: 
after the first calibration the wire broke, and had to be re-wound. 
It must be ascribed to chance, that the deviations are so small just 
at the points of the second calibration. 


§ 6. The jield of utility of the platinum resistance thermometer 
at low temperatures. Resistance thermometers for other fields of tem- 
peratures. The curve in fig. 1 shows at onee the peculiar behaviour 
of platinum below — 200°. At this temperature a change of direction 
in the line which gives the resistance 


as a function of the temperature is 
sharply marked. In fig. 2 the deviations 


from the formula given above in the 
oxygen field are once more represented 
(circles) and also those for the thermo- 
meters (Pt; (squares) and /, (triangles), 
which were also directly compared with 
the hydrogen-ihermometer by Dr. C. 
DorsMan and us. It is clear from the 
curves that we have to deal with a 
specific peculiarity of platinum, which 


Fig. 2. makes it very unsuitable to be used 
as a thermometer in this field, as accurate interpolations ave im- 
possible. For this reason in the field of temperatures below —200°C., 


507 


a gold thermometer is preferable to a platinum one, as has already 
been pointed out by Kamertincn Onnes and Chay '). 

At hydrogen temperatures both platinum and gold are no longer 
approximately linear. Here and at helium temperatures manganine 
and constantin proved to be nearly linear and fit for resistance 
thermometers. Concerning these we refer to a future comm. dealing 
with resistance measurements in particular for the determination of 
the specific heat of mercury at helium temperatures. 

§ 7. Comparison of our thermometer Pty with other platinum 
resistance thermometers. Comparing our measurements with those of 
F. Hrnnina *) formulae of the form: 

aN aN ; 
AR = M(R—1) - N(R—1)? and e' =— M=—— (11000) — 1. 
i : 
were used. This was done because there were objections to a direct 
determination of the temperature coefficient by measuring the resistance 
of Pfr at O° C. and 100° C. which since the first calibration bad 
never been brought to a temperature above the ordinary. We found 


W W 
—— = — 
We W, 
t (K.O. and H.) (Hennine) 10° A R Tel 
= WR INS 0.90523 0.90449 74 0.09551 


43.09 0.82895 0.82775 118 0.17225 
61.50 0.75511 0.75340 alfa 0.24660 
79.57 0.68233 0.67989 237 0.32011 
102.72 0.58822 0.58492 330 0.41508 
113.58 0.54559 0.54007 do2 0.45995 
150.46 0.47389 0.46986 403 0.55014 
182.88 0.25254 0.24686 548 0.75314 
186.79 0.23554 0.22998 556 0.77002 


These numbers give: J/ = — 0.0078758 
N = — 0.0007605. 
And further ¢ = — 0.30.10-° 
100e’ = 0.38821 


From the results it appears that our platinum thermometer, as 
regards its constants, lies between the platinum thermometers N°. 1 
and N°. 7 used by Henning in his investigation. This was to be 
expected, as these thermometers, like ours, were obtained from 
Heranus, N°. 1 and Pr being of earlier date. The difference with 
the values calculated by Henninc is caused by the fact that his 
caleulation was based on our calibration of 1906, which differs from 
our present one and that of 1907 (Comp. § 5). 


1) Comm. N°. 95, Used also by Grommenin, Comm. N°. 140u. 
*) Ann, der Phys. 4te Folge Bd. 40, 1913. 


508 


Physics. -— “On the electrical resistance of pure metals ete. 1X. 
The resistance of mercury, tin, cadmium, constantin, and 
manganin down to temperatures, obtainable with liquid hydrogen 
and with liquid heliwn at its boiling point.’ By Prof. H. 
KAMERLINGH OnnEs and G. Horst. Comm, N°. 142a from the 
physical Laboratory at Leiden. (Communicated by Prof. H. 
KAMERLINGH ONNES). 


(Communicated in the meeting of June 27, 1914). 
§ 1. The resistance of wires of solid mercury. 
Several mercury resistances were compared with the platinum 


resistance thermometer /7/ of the laboratory, first in liquid oxygen, 


| r Wobs. W cate, AW | 

< 4.19 | supra- | 
conductor | 

4.19 0.0560 | 0479 | 0,421 
427 | 00600 |. 0489 ° | 0.429 
4.33 0.0636 | 0.496 0.43 
4.37 0.0656 | 0500 | 0.434 

| 14.57 0.9390 1.667" |) 70,788 

| 15.78 1.069. | 4,806. |" 0787 

hn Eizo 1.298 2.047 ||P o no 
20.39 1563. «S| Ss 2333Ss|CSs.770 | 
80.92 8.086 9.261 1.175 
90.13 9.088 10.316 1,228 

| 116.52 ~ | -2/000,) | * 18.337 9 4).7 seaaan 

| 12281 | 12604 | 14056 | 1.962 
132.72. © | 13800 ~ "|- “15490 1.390 

| 141.83 | 14.855 | 16.233 | 1.278 
154.22 16.354 | 17.651 1,297 
165.80 | 17,806 | 18976 | 1.170 
e402) | “anata en ieies 0.853 
21869 | 24716 | — 25.029 | -O3I8 
233,53 | 26.694 | 26:731. |. 0.037 
234.16 26,800 26.800 =| 0.000 


509 


then at a number of other temperatures, with the differential-galvano- 
meter according to Konnravscu’s method. 

The result of these determinations was as shown in the table (7 = 
temperature on the Ketvin scale, with Zov¢, = 273°.09) 

In the third column are given the values, which would have been 
obtained. if the resistance diminished linearly from the melting point 
down to the absolute zero. 


: seen We tk sae 
Weatc. = — Wy, = —— 26.800 = 0.11445 7. 
ie 234.16 
ts Column + gives the deviations 
w : 
S ool of the real values of the resistance 
us | 4 | | from those, calculated by means 
os 5 , 3 1 ° 
| of the linear formula. These devia- 
ra 4 - tions are also plotted in the figure. 
| | . : 
The relation between electrical 
msg +— : resistance and temperature seems 
to be of a very complicated 
ctl | character. 
aa | 3 § 2. Direct determination of the 
change im resistance at the melting- 
F yebeorse ih \ | point. 


’ 2 1 9 Ee) 9 : é A 
AE aarp Of two resistances, which were 
Fig. 1. frozen without auxiliary bath, the 


change in resistance in melting was determined directly. The first 
consisted of a narrow capillary filled with mercury, section + 0,0015 
mm’. At — 49°.88 the resistance was 25.095 2, immediately above 
the melting point 115.0 2, 
a eh Wa 
the ratio —“ = 4.66. 


Wsol 


The second capillary had a section of 0.48 mm’. With this resis- 
tance the ratio 4.50 was found. 
As a preliminary value of the melting point — 38°.93 C. was found.*) 


§ 3. Indirect determination of the change in resistance at the 
melting point. 

During the numerous determinations of mercury resistances in 
liquid helium (Comm. N°. 133), we always measured the resistance at 
ordinary temperature too. By means of the resistances of solid mercury of 


1) Our measurements date of 1912. In the meantime was published the paper 
of F. Henning Ann, d. Ph. (4) 43 p. 282, 1914 who finds —38°.89 C, 


5LO 


§ 1 and of the well-known behaviour of liquid mercury, we calculated 
lig 
Wsol 


As in these experiments the mercury resistance was suspended in 


in each case the ratio 


a vacuum-vessel cooled from the outside, the freezing took place 
very slowly. 
We found: 
23 May 1914 4.40 


a0) as - 4.63 
WA (OX 3s 4.41 
4.54 


12 Jan. 1912 4.30 wso 


9.06 wys0 


7? Bebrs 4.69 
4.19 
eed; % 4.30 
14 June ,, 4.37 
4.90 


As probably the highest figure thus obtained comes nearest to 
the true value of the ratio, we will be not far from the truth, if 
we assume the number 5 for the mean ratio. 

This result has also been found by Bavrruszaitis'), who obtained 
4.90 as highest value in his melting-experiments. 

It is remarkable, that the ratio of the change with temperature 
of solid and liquid mercury is also about 5; the increase of resistance 
per degree remains thus fairly constant in melting. 


§ 4. Some determinations of the change in resistance with the 
temperature of metals and alloys. 

a. Object of the experiments. We made a series of determinations, 
mainly for orientation, about the change of resistance of different metal 
wires down to helium-temperatures. The purpose of those determinations 
was to find a metal or an alloy, which could be used asa resistance 
thermometer down to the lowest helium temperatures. The results 
of these measurements are plotted in figure 2. Of special interest is 
the behaviour of manganin and constantin. While with copper, tin, 
iron and cadmium no further change of resistance could be established 
in the region of the lowest temperatures, it appeared, that the resistance 
of manganin diminished considerably and in a linear way with the 
temperature, from the lowest oxygen temperatures down to the region 
of the helium temperatures. So that wires of manganin might be 


1) A. Barrruszastis, Cracovie Bull. Acad. Nov. 1912. 


used equally well as wires of constantin (the suitability of which 
was shown on a former occasion), as resistance thermometer in 
this region of temperatures. 

bh. Pure cadmium and pure tin. Pure cadmium (KAHLBAUM) was 
east in a glass tube like mercury. From the tin (KaHLBAUM) a thin 
wire was cut on the lathe. 


t Resistance t : Resistance | 

of tin | of SAE 

| 16.5 | 271.1030 16.6 | 76.7 10-30 

--183.2 | 66.2 | —183.2 209 | 
—201.4 | 46.9 —201.2 | 15.7 
2529 | 2.99 | —252.9 | 1.45 
—258.3 | 1.18 | —258.3 | 0.58 
—268.9 | 0.132 — 268.9 | 0,032 


ec. Copper and iron. The eopper wire was made of commercial 
electrolytic copper’). The iron was from Sweden (Kolswa II). It 


1) W. MEISSNER (Verh. D. Phys. Ges. (16), 262, 1914) used much purer copper. 
In his determinations the resistance at the boiling point of liquid hydrogen was 
only 0.26 °/9 of the resistance at O° C. 


had already been used by Dr. B. Buckman for measurements con- 
cerning the influence of the magnetic field on the resistance. 


| : W copper Wiron 
— 183.7 34.5 3.90 
— 201.7 24.7 3.05 
— 253.5 10.5 2.04 
— 269.5 10.0 2.00 
— 272.0 10.0 2.00 


The resistance approaches here to a definite limiting value, in the 
same way as this has already been found for other not quite pure 
metals (Comm. N°. 119). 

d. Constantin and manganin. The temperature coefticient of con- 
stantin which is extremely small even down to oxygen temperatures, 
increases considerably in the region of the hydrogen temperatures, 
so that constantin wires are suitable thermometers in this region 
and especially in the region of helium temperatures. 


. = 
| | | 


| r Weonstantin Teale. r- Teale. | 
aie Aer 

| 90.75 145.680 

| 65.18 144.320 

| 20.36 | 138,259 20.36 0.00 

| 18.985 | 137.988 | 19.00 | —001 

| 17.33 | 137.662 17.37 | —0.04 

| 15.83 | 137.3555 15.83 0,00 

| 14.32 137.050 14.30 0,02 


yy 


cale ave the values calculated by means of a linear formula of 
the form 
t=a-+ bu 


through the points at 20°36 and 15°.88. The deviation does not 
amount to more than 0°.04 and shows thus the suitability of eon- 
stantin wires as thermometers in the hydrogen region, where the 
platinnm-thermometer would require complicated calibrations (comp. 
Comm. N°. 142c). 


| 4 | W manganin 
| 465C| 124.20 
—183.0 119.35 
—201.7 117.90 
—253.3 | 113.42 
—258.0 | 112.91 
=I G00e met O2 
Sie es Ghul 


e. Gold. With a view to measurements -of specific heats, which 
will be published before long and to investigate the suitability of the 
‘gold-thermometer in the region of oxygen- and hydrogen-temperatures, 
we determined the resistance of a gold wire at a great number of 
temperatures in those regions.') The result shows, that in the region 
of the reduced-oxygen temperatures (mainly below — 200° C.) the 
gold thermometer does not give rise to the difficulties, which make 
the platinum thermometer nearly worthless in that region (Comm. 
N°. 141@ § 6 and tig. 2). 


| T Resistance | 


of gold 
1418K 0.2910 
15.83 0.3037 
17.30 0.3190 
19,00 0.3412 | 
20,35 0.3621 | 
65.18 | 2.2901 | 
| 72.58 | 26763 | 
83.31 3.2312 
87,99 3.4710 
90.75 3.6110 


1) Calibrations of other gold wires will be given in the paper by W. H. Kersom 
and H. KAMpRLINGH ONNes on specific heats Comm, N°. 143, 


514 


Physics. “Further experiments with liquid helium. L. The persistence 
of currents without electro-motive force in supra-conducting 
circuits.’ (Continuation of J). By Prof. H. Kamerinen OnnEs. 
Communication N°. 1416 from the Physical Laboratory at 
Leiden. 


(Communicated in the meeting of June 27, 1914). 


§ 9. The preservation af an electro-hinetic momentum. All the 
phenomena that were dealt with in the preceding sections (J) *) 
showing the persistence of the magnetic moment of the coil, 
without the acticn of an electro-motive force, agree with what was 
deduced on the supposition that a enrrent flows through the coil of 
the value calculated, and which diminishes according to the time- 
of relaxation calculated. At the same time, it was desirable to have 
a conelusive proof that the magnetic moment of the coil is really 
caused by a current. We should then be able to prove conversely 
by the continuation of the moment, that the time of relaxation of 
the current is very long, and a value, or otherwise an upper limit 
could) be given for the micro-residual-resistance of the conduetor in 
which this current flows. 

I got this proof in the following manner. 

On either side of the place, where the ends of the windings of 
the coil are sealed together and close to it, two wires b, b (see 
fio. 2 and 1) were fixed which lead to a ballistic galvanometer. 
Between these points of attachment the current can be cut through 
under helium, by pulling up by a thread a bronze loop provided on 
the inside with a knife edge at m (see figs 3 and 1. Figs 1 and 2 give 

1) Disregarding the existence of threshold-values of current and field and consi- 
dering that, below these, supra-conductors add up algebraically without appreciable 
loss the inductional impulses which act on them in the course of time, two points 
of view may be very simply contrasted in connection with the experiments so far 
described on the production of currents persisting for a long lime. 

The first is analogous to that taken up in Weser’s explanation of diamagnetism. 
In this case we deal with supra-conducting circuits which are currentless outside 
the magnetic field. By bringing these into a field currents may be oblained which 
persist as long as the field remains unchanged. But when the field disappears the 
circuits become again free of current. In this manner a good imitation is obtained 
of diagmagnetic polarisation. The other point of view may be called the antilo- 
gon of that of Weser. We provide in a magnetic field’ supra-condueting cireuils 
which are free of current. When these circuits are brought outside the field, they 
show a current persisting for a long time. Outside the field they imitate permanent 
magnets. It, must, however, not be lost sight of, that. this imitation is in so far 
incomplete, as when the circuits are brought back into the field, they return to 
the currentless condition. 


S18 


a combined view of the experiments of sees 
tions 9 and 11). The thread runs through a 


2 Sk eee mee 
4 tube, the lower part of which is of glass and 
can be moved by means of a rubber-tubing 
calles attachment at the top of the apparatus (fig. 1). 


The coil was cooled to 2°.4 K. in a field 
of 200 gauss by helium evaporating under 
reduced pressure. The current was again 


produced through induction by removing the 
field. When the compass needle with the com- 
pensation-coils was arranged, as before, beside 
the cryostat, a moment corresponding to a 
current of 0.36 amp. was registered. The 
observation was continued for an hour, in 
which the diminution of the current in 45 
minutes was within the limits of probable 
error of the measurement (2°/,); after this 
the circuit of the coil was cut through. The 
(| needle of the compass fell back to a deviation 
| that corresponded to a current of 0.05 amp. 
in the coil. The ballistic galvanometer (with a 
negligible self-induction and with 2000 2 in 


Fig. Fig the circuit) showed an electro-kiretic momentum 
2. 3. Lj of 300000, from which follows with L—10', 
that a current of about 0.8 amp. flowed in the coil. The remaining 
moment is again the same fraction of the principal effect as was 


observed previously, it was extinguished as soon as the coil was 
pulled up above the liquid helium. The experiment proves conclusively, 
that a current does really flow through the coil. 


§ 10. Further consideration of the momentum produced in the 
coil, when the circuit is not closed. Persisting Foucauiy-currents. In 
the previous experiments the question arose in how far magnetic 
properties of the frame of the coil, which developed at the lowest 
temperatures had an influence, and whether a part of the moment 
that remained, when the coil, without the ends being connected, was 
cooled and exposed to the field, was due to windings which were 
short-circuited. For this purpose first of all a tube of brass, exactly 
like that used as the frame of the coil, was cooled in the field. 
It showed no residual magnetism. 

To get further light on possible short-cireuits in the coil Phx, 
after it had been shown that cooling in liquid air did not alter 

ot 

Proceedings Rayal Acad. Amsterdam. Vol. XVII. 


51 


iis moment, a new coil of 650 turns was wound, in which the 
possibility of short-cireuiting was excluded by insulation of the 
windings by picein ani paper. It is true that the magnetic 
properties of these materials are not known, but from the extinction 
immediately above the boiling-point of helium of persisting current 
which was found in the course of the experiments it is almost certain, 
that the phenomena are entirely due to the lead. It was ascertained 
that this coil was superconductive, which was a welcome result also 
for the reason that the wire had been manufactured by compression, 
and this process gives a much better guarantee of getting the same 
product again by using the same method, and therefore of obtaining 
beforehand the certainty of the wires prepared in this way being 
supra-conducting. In making the experiment with 200 gauss at 2°.4 K. 
a residual effect of the same order as with Pbx7;; was found, but 
smaller. The principal current was 0.5 and the residual current 
0.020 Amp. It becomes probable, when these figures are compared 
with those found with Pbx,7,, that in the latter there really is some 
short-cireuiting, but there is also apart from the effect due to the 
short-circuited windings a moment caused by the lead. 

It seems as if in the mean time this may be attributed to circular 
currents in the lead of the wire, which are possible owing to the 
wire having a certain thickness. We must distinguish in the wire 
between an inside which is turned towards the axis of the coil, 
and an outside. In the wire, even when the circuit is opened, a 
current arises, in which the electricity passes along the whele 
length of the windings on the outside of the wire (that is not closed 
in itself), in order to turn round at the one end of the wire and 
go back along the internal side. With induction in the closed cireuit 
this current is superposed upon the mean electric movement in 
the cireulating current, so that in the wire there is say a stronger 
current on the outside, and a weaker on the inside. If by means 
of a galvanic cell a current is sent through the wire, the same 
phenomenon arises through the action of the field of the current 
itself. We are here evidently dealing with persisting Foucaun- 


currents '). 


§ 11. A supraconducting key. In the experiments so far de- 
seribed the supra-conducting closing of the conductor tested for supra- 
conductivity was obtained by melting the two ends together. Now 
1) Several of the well known experiments by Exinu Tuomson with alternating 
eurrents could also be made with parallel currents and supra-conducling experi- 
mental objects. 


517 


that these experiments had proved that a current generated in a 
circuit which is supra-conducting over its whole length, continues 
without electro-motive force, we could investigate in how far an 
electric contact interposed in an otherwise supra-conducting circuit, 
measured by the amount of conductivity of supra-conductors, might 
be considered as having no resistance. The immediate cause of this 
investigation was a suggestion made by my colleague Kunnnn, whether 
the current the relaxation period of which was to be studied, 
might not be obtained in the coil by short-cireuiting. 

I thought then, that the transitional resistance in a contact to 
be manipulated under liquid helinm could hardly be made small 
enough for this purpose. The transitional resistance of a stop- 
contact treated with all due care at ordinary temperature is not 
likely to be less than 0,0001 2, which is still 100,000 C.G.S. while 
the micro-resistance of the coil itself is only 37. It has now been 
found, however, that transitional resistances such as we are con- 
sidering can become very small at low temperatures. A quite moderate 
pressure, between two pieces of lead appeared to be sufficient for 
the purpose. The arrangement is shown in Fig. 2. The small lead 
plate p, provided with three small cones direeted upwards and 
connected with the coil through a spirally-wound part of the lead 
wire which acted as a spring, is attached to a thin rod (partly formed 
of wood) and was pressed against the block soldered to the glass tube 
by serewing up the rod, the force being accurately regulated by means 
of a spring (see top of fig. 1). The tube is provided with a number 
of side-openings to prevent the very much intensified heat convec- 
{ion (caused by resonance phenomena) which occurs in tubes closed 
at the top when the bottom is at a very low temperature, and 
which would lead to excessive evaporation of the helium. 

Ry means of this simple key we were enabled to arrange the 
following experiment. To each extremity of the windings of the coil 
two wires were attached (fig. 1 and 2). By means of the one pair ac a 
current can be sent through the coil. The other pair 6 can be con- 
nected toa ballistic galvanometer. Moreover the two ends are connected 
to the two parts of the supra-conducting key. With the key and the 
galvanometer open, a current is sent through the cooled coil, in 
the neighbourhood of which the compass-needle has been mounted. 
The coil is then closed in itself, which gives no change in the 
deviation of the needle. One ean then convince oneself as long as 
one likes, that the side-current, which in ordinary cases is imme- 
diately extinguished, remains unaltered in the supra-conductor; the 
galvanometer connection is then closed, which also brings no change 


34% 


S18 


in the current, and if thereupon the current connection is opened 
this is accompanied by a throw of the ballistie galvanometer in the 
circuit of which the current is instantly extinguished and by a return 
of the needle of the compass into the position which it would also 
take up, if the current in the closed coil had been generated by a 
magnetic field equal to that of the current itself. The continuation 
of the movements in Maxwenr’s mechanism, when it has a supra- 
conductor as carrier, is demonstrated by this experiment with equal 
clearness and simplicity. 


§ 12. Combination of parallel currents into one of greater strength. 
In trying to make the same experiments with mereury that we have 
made with lead, it will be necessary in so far to change the experiment, 
that one winding will be sufficient. This might be got by. freezing 
mereury in a capillary tube returming in itself with an expansion 
head (like our other U-shaped mereury resistances). The chief 
questions then are 1) if with a conductor of as large a section (keeping 
for the present to the circular form) as would be necessary, with a 
view to the threshold value of current density, in order to get an 
action comparable to that with the lead coil, the threshold value of 
current density — of which as in N°. 183 if is assumed that it is 
determined principally by the current density —— does not undergo 
a considerable diminution in consequence of the larger section, as 
some considerations in N°. 183 would make us fear, and 2) if we 
ean reckon with the microresidual resistance as an ordinary resist- 
ance even for such a completely different section as that for whieh 
it has been determined. An inducement to try the experiment imme- 
diately with a lead ring*) was a remark by my colleague Enreneest, 


1) f am glad to mention here that Mr. J. J. Taupin Caasor of Degerloch 
(Wiirttemberg) shortly after my paper on the disappearance of resistance in mer- 
cury and, as I found afterwards, only acquainted with my result, that the resist- 
ance of gold and platinum in an absolutely pure condition would probably disappear 
allogether at extremely low temperatures, communicated to me a number of suggest- 
ions regarding the condition into which meta!s pass below this temperature and 
which he would like to be considered as a distinct “fifth” state of aggregation. 

Amongst these suggestions was the following: “if a ring (of gold) is brought 
to the condition of absolutely no resistance (in helium), an impulse (viz. by im- 
duction) will be sufficient to produce a permanent current, which will make the 
ring into a magnetic shell, as long as the temperature of the metal remains below 
a certain critical value”. By critical value was meant — nol the vanishing point 
as discovered afterwards — but the temperature characteristic of each metal at 
which, according to my earlier views, the resistance of the pure metal would 
become zero independently of the current-strength. The idea, however, underlying 
this speculation — which was further developed by supposing the cooled ring to 


519 


that the experiment could be made equally well with the windings 
“parallel” as it had been made with the windings in “series”. A 
calculation (by estimation and further proceeding in the same way 
as with the coil) about the experiment with a lead ring of an internal 
radius of 1.2 em. of a thickness of 0.38 em. and of a width of 
0.35 em. and assuming that the threshold value found for the thin lead 
wire would also hold for the thick ring, showed me, that it might 
sueceed very well.’ 

This proved to be the case. The current of 320 amp. that was 
registered in the ring remained constant for half-an-hour to 1°/,, hence 
the current density of 50 was in this experiment not much smaller 
than it had been in one of the experiments with the coil of lead 
wire, viz. 49. This may for the present be regarded as a confirm- 
ation of the supposition that the thresbold value of current strength 
of a conductor is mainly a threshold value of current density for 
the material of the conductor. 


be subjected to a magnetic field which was to be removed afterwards — was also 
applied in my experiments for the purpose of obtaining persisting currents in supra- 
conductors, and in the above last experiment actually with a ring as the conduet- 
ing circuit. 

At the time I was so much occupied with the investigation of the peculiar laws 
of electric conduction in mercury below the vanishing-point and of the degree to 
which currents miglit be realised in resistanceless circuits without electromotive 
force, that I had not yet attacked or was able to fully go into the problems relating 
to currents to be generated in closed supra-conductors by induction (amongst which 
proklems that of the imitation of diamagnetic polarisation was an obvious one). 
Still Mr. Taupin Cuazor’s letter was the cause of my coming even then to the 
conclusion, that in order to be able to obtain persisting currents outside the magnetic 
field by induction, an artifice based on the peculiarity of supra conductors was 
required. As such I then found, that the cooling which is to make the conductor 
supra-conducting is not applied, until the conductor is in the field which 
is to be used for the induction. Afterwards it was found, that by utilizing the 
knowledge of the threshold values of current and field circumstances may be realized, 
in which a permanent current may be obtained outside the field by induction on 


a circuit which has been made supraconducling by cooling before the field is applied. 


520 


Physics. — ‘“/urther experiments with liquid helium N. Waut-effect 
and the change of resistance in a maynetic field. X. Measure- 
ments on cadmium, graphite, gold, silver, bismuth, lead, tin 
and nickel, at hydrogen- and helium-temperatures. By Prot. 
H. Kamerrtincn Onnes and K. Hor. (Communication N°. 1424 
from the Physical Laboratory at Leiden.) 


(Communicated in the meeting of June 27, 1914). 


§ 1. Method. The method was the same as that used in the 
measurements of this series by H. Kamernincn Onnes and BuckMANN 
‘ef. Comm. N°. 129a and others). The notation is also the same as in 
the previous papers. As regards the HA.t-effect, we used both the 
method in which a galvanometer-deflection caused by the effect’ is 
read and the compensation-method, in view of the fact, that the 
latter, althongh in general to be preferred, as it allows the elimination 
of various disturbances, is very troublesome, when small effects 
have to be measured. The differential-galvanometer used was of the 
Kervin-pattern with a volt-sensibility of 5 >¥ 10-8 ; it was iron: shielded 
and was mounted according to Jurius. As to the resistance measure- 
ments these were partly performed in immediate connection with 
the determination of the Haxt-effect, in which case the resistance 
of the plate used for this purpose was at the same time measured, 
partly (by means of the compensation-apparatus) with wires which 
were wound on thin sheets of mica and could be placed either at 
right angles to the field or parallel to it, the latter specially with 
a view to investigating the considerable difference between the trans- 
verse and the longitudinal effect, which difference develops specially 
at helinm-temperatures. 


§ 2. Sismuth. In accordance with frequent practice (e.g. by 
KAMERLINGH ONNES and BrckKMANN) we used this substance in the 
form of pressed plates. The peculiarities in the resistance observed 
by Srrewntz with conductors of compressed powder — although 
occurring also in our plates at higher temperatures were not 
observable, when the plates were cooled below 0° C. 

The plates which served for our investigation were pressed in a 
steel mould and heated to about 200°C. in an electric furnace. 
When made in this way the granular structure was still clearly 
observable with a magnifying glass. The plate ip; was made 
without special precautions; with plate iyz, the metallic powder 


521 


was specially dried before moulding it. Diy; gave an abnormally 
high temperature-coefficient at higher temperatures and even after 
36 hours’ heating had not yet attained a constant resistance. 

The metastable condition which according to Professor E. Conrn 
is peculiar of most metals as mixtures of different modifications 
manifested itself also in our experiments. The plates after being 
heated in the electric furnace to 60° or 100° C. showed some dif- 
ference as regards resistance and Hatt-effect after cooling, with the 
further peculiarity, that this change fook place, although no change 
in the specific gravity affecting the second decimal place could be 
established. 

The results are contained in tables I and II. 


TABLE I. 
; | 
Biy,- | 
H —R Resistance —R | Resistance | 
} | | 
| T=2899° K | T=20°5 K | | 
2400 Gauss | 7.71 | 2.5°10-3 Serato 
2420, 42.13 
4800, 6.68 Is 22385958 
i200); 4 6.02 35.44 | | 
9650, | 5.37 | 3862 
| | | if 
11800, | 29.76 | 1.1°10-3 | 
| 
12000, 4.65 | 3.1°10-3 QO) | 
TABLE Il. 
Biyyy 
H —R Resistance —R Resistance | 
T=289° K T=20 K 
2420 Gauss 10.57 2.4.10-3 80.03 3.10—-4 
4800, 9.48 | 78.31 
1200'= 5 8.11 | 75.15 
9650, 7.26 72.51 | 
12000, 6.28 3.2.10-3 | 70.82 | 1.6.10-3 


522 


§ 3. Hant-effect in graphite. The great change in the properties 
of graphite through even small admixtures appears clearly from the 
fact, that with different kinds of graphite the temperature-coefficient 
of the resistance may even differ in sign. 

The material we started from in our experiments was fine graphite- 
powder, such as is used in electro-plating; the powder was first 
treated with acids and alkali and carefully dried; the forming of the 
plate was again carried out in a steel mould. The electrodes which 
gave some difficulty at first were finally contrived in the following 
manner: the powder was provisionaily moulded to a plate under 
comparatively low pressure, the stamp was then lifted off and six 
small pellets of solder were laid on the plate, after which a high 
pressure was applied. By trial we succeeded finally in obtaining 
suitable plates of */; mm. thickness with six point-electrodes of about 
‘/, mm. diameter, penetrating through the whole thickness of the 
plate. 

The influence of insufficient drying of the powder was very 
marked; such plates, as did not come up to standard as regards 
drying, did not reach their final resistance until the current had 
gone through for 6 seconds. 

The following table contains the results. It may be specially noted 
that the ftemperature-coefficient is positive and that the Hats-effect 
falls strongly from 20° K. to 14° K. 


TABLE III. 
Graphite. 
H 290° K 20°.5 K 14°.5 K 
aes ee 
+R: +R: +R: 
| 4800 Gauss | 0.68 3.4 1.42 
6000, 0.68 
4200: te 3.39 
8400, 0.68 1.52 
96005 aa 2.81 
11800, 0.74 2.22 1.52 


§ 4. The Haut-ejject in cadmium. Two eireular rolled-out Cadmium- 
plates of 1 em. diameter were experimented on, The results are 
found in the following table. 


TABLE IV. 

| Cadmium. 
| areas | eae | : | 
| H | 2O0OT Ke se 20e owke | 149.5 K 
| + R: \Neeeesce | +R: 
| 3000 Gauss | 13.1104 | 

2600 ye 4.6.10—4 | 

4800 ot, tt e202 OSA eens Oe 

6000, 6.3.10—4 | 

7200 + 20.6.10—4 | 23.4.10—4 | 
3400) 5.9.10-4 
| 9600 : 19.6.10—4 | 22.3:10—4 | 
| 11800 " LWie6.1054> | 191105255) 
| 12000 4, | 5.5.10-4 | | 


§ 5. The Haut-ejiect at helium-temperatures. The method was the 
same as in the previous measurements. To check the results, measure- 
ments were made both with the compensation-apparatus and with 
the differential-galvanometer. Five different plates were experimented 
upon in the helium-bath. These were chosen so, that they could be 
regarded as representatives of metals for which the Hat-effect is of 
a different type. Each set of six wires from the six electrodes of 
one plate was completely separated from the other sets in the cryostat. 

The following plates were investigated. 

1. A tin and a lead plate: both metals are supra-condueting at 
extremely low temperatures. Lead remains supra-conducting up toa 
considerable threshold-value of current. It may be added that both 
are diamagnetic: as pe Haas has shown, the diamagnetic properties 
are of great importance for the Ha.u-effect. 

At hydrogen-temperatures the Hatu-effect is still so small, that it 
escapes observation. It was found that at 4°.25 K. both with tin 
and lead the effect can be very well measured, when the field is 
so high, that ordinary resistance is generated in the metals. As long 
as the field is low enough for the metal to remain supra-condueting, 
the Haut-effect, like the ordinary resistance, disappears. 

2. A silver plate, as representative of the group of metals for 
which at the ordinary temperature the Haz1-coefficient is of the 


524 


TABLE V. 


Measurements in Helium. 


H R 
| 1. Sr (tin) | 
Lane acs KK | 
11300 Gauss + 2.6.10—5 
Owe COn + 9.8.10—5 
2. Pb (lead) 
A. AZO 
300 Gauss < 6.10-5 
1000, < 2.10-5 
5000, -+ 0.8.10—4 
11300, + 1,8.10-4 
BIO OR 
300 Gauss < 6.10-5 
11300 Si, + 1.3.10—-4 
3. Ag (silver) 
a. T={4925 K 
11300 Gauss 16.10—4 
b. T=2°S K 
13000. 16.10—4 
4. Ni (nickel) 
a. T= 4925 K 
1300 < 5.105 
11300 <— Wet0=5 
Ox i= 228K 
11300 <<) OSs 
5. Bi 
TANK | 
1000 Gauss | 86.3 
5000, in = | 84.2 
11300, 85.7 


order of magnitude 10—4; silver is diamagnetic and does not become 
supra-conducting at helium-temperatures. 

As appears from the table, it was found that with silver also the 
Hati-effect increases, when the temperature falls to 4.925 K. At 
still lower temperature it does not show any further change, no 
more than the resistance without a field. 

3. A bismuth-plate B/y7,;, moulded from electrolytic bismuth- 
powder. Bismuth has a very high Hant-effect at hydrogen-temperatures 
and the change from 20° K. to 14° K. is still very small. It is the 
strongest diamagnetic metal. 

The table shows that below 14o K. there is not much further 
change in the Haut-effect. From 71 at 20° K. & rises only to 85 
at 4°.25 K. 

4. A nickel plate as representative of the ferro-magnetic metals. 
With nickel at higner temperatures the Hatt-effect shows a tendency 
to saturation owing to the magnetisation of the metal (Comm. No. 129, 
130, 132). At hydrogen-temperatures the effect is still easily measu- 
rable; at helium-temperatures it disappears, although the resistance 
of the plate is still considerable. Probably this is connected with the 
fact, that notwithstanding the already fairly considerable field the 
magnetisation of the nickel is still very small. 

The results are collected im table V. (zie p. 577). 


§ 6. Change of the resistance in the magnetic field. It was found, 
that specially at helium-temperatures this change is very con- 
siderable, but that at 20° K. also it is still quite well measurable. 
In general there is a difference between the longitudinal and the trans- 
verse effects, which begins to show itself especially clearly at helium- 
temperatures. 

We shall give our results in the form of curves (figs. 1 to 6) on 
which the numerical values may also be read with sufficient accuracy 


by using the scale-values indicated in the figures. So far thé meas- 


28. co T i if [ieee (a 3 T Bea 
29% + ———_-|—_ ee ee = =a | a eo = — 


A | 
fore os eee eae { = a 4 |} =e 
ie a | | 
191.1 ad lie 245 = = == =k 
a 2000 yoo. dan C000 10000, moo 


(yams. 


526 


urements both at hydrogen- and helium-temperatures have not gone 
beyond 12000 Gauss. They will afterwards be further extended to 
higher field-strengths especially at hydrogen-temperatures. 


40S 127 


"7 


Figs. 1 and 2 contain the results for the resistance of lead and 
tin in a magnetic field. The difference between the longitudinal and 


- > , . 
aot7s syiolizitce Caio viv 1091. 
1 


Sa eral! 


aoz23s. }— 


oO £000 4000 do0a. e000 10000 12000 
> 
Gauss 


Fig. 3. 


transverse effects was not more than the errors of the measurements. 
The abscissa gives the ratio of the resistance to that at 0° C. 


2 
Goss ] T | 
> . pian 
aos} 4 MNeoistance Mla tisrii ya 


00381 


aos4 }— 


° 
yamss 


527 


Fic. 3 and 4 represent the longitudinal and transverse effects 
o | to) 

for cadmium and for platinum. The abscissae give directly the 
resistance in Ohms. 


as 


a Ja toa 190 100 t30 300 Dt 


Fie. 5 and 6 show the results for graphite, Fig. 5 the dependence 
of the resistance on ihe temperature, fig. 6 the dependence on the 
magnetic field. 

We have further made measurements on the resistance of a 


Bicgane | 
1 ak el 


cy wat pbite. = ieee 


e000 wove. 1x00 


a) 
Fig. 6. pice 


plate of not-purified graphite. These are not concluded, however, 
and will be published later together with measurements on polarisa- 
tion-phenomena which may possibly show themselves with pressed 
graphite. 


598 


Physics. — “Measurements on the capillarity of Viquid hydrogen”. 
By H. Kamerninch Onnes and H. A. Kuypers. (Communication 


N*. 142d from the physical laboratory at Leyden). 


(Communicated in the meeting of June 27, 1914). 


For the determination of the capillary constant of liquid hydrogen 
in contact with ifs saturated vapour the method of capillary rise was 
used. The apparatus are in the main arranged in the manner as used 
for other liquid gases in Comm. N°. 18. On plate IA of Comm. 

N°. 107a@ may be seen that part of the apparatus 
which serves to condense the gas in the wide 
experimental tube (fig. 1), inside which is the eapil- 
lary ; for this purpose the tube of fig. 1 is sealed 


— - Sty. in at g,. 
The radii of the sections of the tubes were found 
by calibration with mercury as follows : 
radius of the capillary inside 7 = 0.3316 em 
3 Sere, 3 outside 7, = 0.0801 em 
¥ » >», surrounding tube inside = 0.554 em 
Measurement of the capillary rise. The reading 
of the ascension gave some trouble as it had to be 
made threugh a number of glass vessels and baths. 
The rise was measured with a eathetometer ; to test 
the accuracy of the readings they were taken one 
{ime on a millimetrescale which had been etched 
Fig. 1. on the capillary and another time directly on the 
scale of the cathetometer. When it was found, that there was no 
difference between the heights obtained in the two ways, they were 
afterwards only measured by means of the scale of the catheto- 
ineter, because, when the eryostat was filled with the different liquid 
gases, the divisions on the capillary were difficult to distinguish owing 
to the rising gas-bubbles in the liquids. 

Temperature. The temperature was deduced from the pressure of 
the vapour in the hydrogen-bath using the vapour-pressure curve 
(H. Kamerninco Oxnes and W. H. Kersom, Comm. N°. 137d. table 
on page 41). 


Observations. The heights measured and the corresponding tem- 
peratures of the hydrogen are contained in the following table, 


529 


Repeated measurements show, that the accuracy of the reading of 
the rise may be estimated at 0.002. 


TABLE I. 
| Temperature in | Rise 
KELVIN-degrees | in cms, 
[is A See See 
20.40 | 1.616 
18.70 1.794 
17.99 1.869 
16.16 | 2.064 
14.78 | 2.209 


The observed heights (4) have to be corrected for the curvature 
of the surfaces by means of the following formulae : (1) the correction 


. ib s . . 
for the meniscus in the narrow tube is a ‘). (2) the correction for 


the ring-shaped meniscus is (according to VerscHarreiT Comm, N*. 18). 


: ipa 2 
w=(1 -f ar (k =. 


> (R—?,) 


For this correction the height of the ring-shaped meniscus, as the 
minor axis of the elliptical section with a meridian plane, is required 
to be known. With the illumination used this height could not be 
measured accurately. Afterwards for further correction we hope to 
be able to determine its value by special measurements: in the 
mean time the section was assumed to be circular with sufficient 
approximation. The corrected values are given in column 6 of table II. 

When the capillary rise is plotted as a function of the temperature 
— fig, 2 —, a straight line is obtained. The constants determined 
from this line give the formula 

H= — 0.1124 7 + 40.44. 


This formula gives H=0 for T'y7=0 extray. = 35.98 K. 

Assuming the critical temperature to be 7), —= 31.11 1 (mean of 
1) Laptace, Méc. Cél. Tome X, Supp. § 5, Paris 1805. 
id. , Oeuvres Tome IV, p. 415, Paris 1845. 
Attan Ferguson, Phil. Mag., p. 128, (6) 28, 1914. 


530 


oie 
24 aS 
35 | \ 
R 
2.2 - x 
NN 
\ 
\ 
29 XS 
: ® 
19 < 
Ht 
1,8 
7 1 he J I = 
‘ 1S 6 ” 8 19 £0 % 
- Fig. 2. 


Drwar, Oszewski and BuLir)') it is seen, that the formula, as was 
to be expected, does not hold up to the critical temperature and 
that the curve which gives the dependence of // on the temperature 
has its concave side towards the temperature-axis. The difference 
T'H=0extvap.— 7, for hydrogen amounts to 


T 77=0 extrap. — Lito eOits 


If Vry—oextrap. — 77. is divided by the critical temperature the 
I 4 | 


3.87 


positive value = 0.125 is obtained. For methyl-chloride*) and 


ethylether*) similar values are obtained *). 
Surface-tension. From the capillary rise the surface-tension yw, is 
found by means of the following formula : 


2, 1 1 
i NET vr (- — az) 
(tig. a! Ovap.) ANGE R =n 


The densities for liquid hydrogen are taken from the observations 
by H. Kamerninca Onnes and C. A. Crommetry (Comm. No. 137). 


1) F, Burnie. Physik. Zeitschr. p. 860, XIV, 1913. 

*) According to measurements by J. VeRSCHAFFELT; comp. A. v. ELDIK, 
Comm. N°. 39, p. 14. 

3) E. C. pE Vries, Comm. N°, 6. 

4) The corresponding figures (deduced, however, from not-corresponding tem- 
perature ranges) are 9.038 and 0.017 respectively. 


531 


For the calculation of the vapour-densities use is made of the second 
virial coefficient, as deduced from the measurements by H. KamErLiIncH 
Onnes and W. J. pe Haas (Comm. No. 127c). 


| 
| 
{ 
{ 
| 


| 7 = 3332 3 2 
dD — eet SS eS) = 
l SS. S25) Oi S2' Sk 1S 
| & St WRehit hatte peices 
West) panel eae taal ate 
> 
rec ae 
@& |@&a 8 BER B® 
6 & = = Ss OF ITD 
COR Sn ecg i i 
ie = QIN EN AW I a con cd 
oe eal 
o | 
S || 10 16 0 
“a 
oa yen Cy SG Nil er eS) 
| lmaeterenatrenentroy “al hse alse 1 
. || eres 
AS | © 
o 
: Gere eel Gel oh ev Tse) Kat) 
&. Seo) St ON TO Os IO 
ze S 
wT oO 
= = im 10 
4 CO = O) 00) Oecd Pe SE oH 
o SS 1S) Qs ies)! Wo o 
aa 4 LeSieg USaS  ly ile Lah lah sal Soe 
— oa oS | 
faa) = —— 
< | 19 
[= — Cy oy OT 
= Ste NO AOy a SHC cor =) (00) 
ee Wi eS ES ey SS Gai Ge) 
om NNON NN 
i 
ov o | 
<= ro IN A tts et C= 
= Sn | eens Us CCR CON SHE IOI COMO) 
a QA | a Se Se Se ea BSB Se 
23) 3 S 
i>} 
SQ | | — 
Ore | 
So | 
met |S) ba ee ee 
2 MS) Ss SS SSS SS 
m 
3 2 
oO a oS 
ie] 
CO Tos oy sta a 
= =- = = &® © & DB S 
OO OR) 00 OS a ic 
| J= ae we ae =z nna 
| 
4 
| Qa, Ol any: 19 
& io ee OC &) © ey ce) 
3 {Vibe Seay ites Sines eee 
= =) te fey ee) Te ke 
N A AN Hee me Oe 


With these data the values of yw, in table II are calculated. Under 
O—C are given the differences between w, ops, and values of yp, caleu- 
lated from vAN per Waats’ formula 

w= A(1—p2 
where 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


532 


A = 5.792 
B= 0.9885 

From the value found for B it appears, that y, as a function of 
T is nearly a straight line. 

The constant in Eérvés’ formula for hydrogen deviates considerably 
from the value 2.12, found by Ramsay and Surrips ') as the average 
for a number of normal substances. In Table ITI the values of ps 
for a few of these substances, together with those for some liquid 
gases, are collected. As observed by KameriincH Onnes and Krgsom 
(note 3881 Suppl. No. 23), normal substances form a series in this respect, 
on the whole progressing with the critical temperature (although with 
deviations which may be ascribed to particularities in the law of 
molecular attraction, e.g. with oxygen). 


TABLE Ill. 
| Ethylether ) Pi ey 
Benzene 2) 2.1043 
| Argon 3) 2.020 
| Nitrogen 3) 2.002 


| 
| | 
| Carb.monoxide3) 1.996 


| Oxygen 3) | 1.917 
_ Hydrogen | 1.464 


A calculation of the constant 4’ in Ersrer’s formula ‘*) 


dw, 2 
ip — LF jos Sk Api RL 
i(« dT ) "Tig. I Oe AAG 


for hydrogen gives 
7.34 < 107 
The fact, that hydrogen appears to have a considerably higher 
value of 4’ than that calculated by Erystrein for benzene, might, in 
view of the theory underlying the formula, indicate, that the radius 
of molecular action is larger for hydrogen molecules than for sub- 
stances like benzene. 


\) J. chem. Soc. 63 (1893); ZS. f. physik. Chem. 12 (1893). 

*) Ramsay and Surexps ZS. f. physik. Chem. 12 (1893), 15 (1894). 
8) Baty and Donnan, Journ. chem. soe. 81 (1902). 

4) A. Etnstern, Ann, d. Phys. 4. 34, 1911. 


533 


Chemistry. — “The system: copper sulphate, copper chlorid, potas- 
sium sulphate, potassium chlorid and water at 30°”. By Prof. 
F. A. H. Scurememakers and Miss W. C. bE Baar. 


1. Introduction. 


In previous communications ') we have discussed the quaternary 
systems: 
Cu SO, — Cu Cl, — (NH,), SO, — NH, Cl — water 
and CuSO, — CuCl, — Na, SO, —NaCl — water 
Now we shall discuss the system 
Cu SO, — Cu Cl, — K, SO, — KCl — water, 
which we have examined at 30°. 
As solid substances occur at 30°: 
the anhydrie salts: K,SO, and KCl, 
the hydrates: CuSO,.5H,O and CuCl, . 2H,0, 
the doublesalts: CuSO,.K,SO,.6H,O and CuCl, : 2KCI. 20,0. 
Further a peculiar salt exists with the composition : 
Cus@, kK Cl or K. sO, Ca Cl, 
with or without one molecule H,O, while sometimes as metastable 
solid phase a salt with the composition : 
2CuSO, . 3K,Cl, . H,O 
has occurred. 
In fig. 1 the equilibria occurring at 30° are represented schematic- 


G. SO, 


222 (1911) and Zeitschr. fiir Phys. 


Chemie 69, 557, (1909). 


35* 


5384 


ally, the sides of the quadrangle have been omitted, only a part 
of the diagonals with their point of intersection W is drawn. Fig. 1 
is not the representation in space of the equilibria, but thew pro- 
jection on the quadrangle. Before discussing the quaternary equili- 
brium, we will first consider the four ternary equilibria. 


2. The ternary equilibria. 


a. The system K,SO,— KCl— H,O. 

Only K,SO, and KCl occur as solid phases; in fig. 1 the satura- 
tioneurve of K,SO, is represented by Ag and that of KCl by /g. 
Consequently point ’ represents the solubility of K,SO,, point / the 
solubility of KCl in water; point g is the solution, saturated with 
the two salts. 

b. The system CuSO, — K,SO,— H,0. 

This system was examined already formerly *); as solid phases 
occur K,SO,, CuSO,.5H,O0 and the doublesalt CuSO,.K,SO,.6H,0. 
The isotherms of 80° and 40° are determined experimentally ; that 
of 30° is represented schematically in the figure. The saturation- 
curve of K,SO, has been represented by /z, that of CuSO, .5H,O 
by ak and that of the doublesalt by 47. When we represent this 
doublesalt in tig. 1 by the point D,.,., then the line WD,.,., intersects 
the curve 7k in a point 7. The doublesalt is, therefore, soluble in 
water without decomposition; its solution saturated at 30° is repre- 
sented by 7. 

The following is still of importance for the investigation of 
the quaternary system. When we heat an aqueous solution of 
K,SO, + CuSO, above 50°, a light green salt is separated from the 
solution. Mrrrpure found for the composition of this salt: 

4CuO . K,O .. 450, . 30,0, 
while Brunner’), who examined first this basical salt has found 
four molecules instead of 38 molecules H,O. 

c. The system CuSO, — CuCl, — A, 0. 

Also. this system was investigated formerly *), as solid  sub- 
stances occur: CuSO,.5H,O and CuCl, .2H,O. In fig. 1 ab represents 
the saturationcurve of CuSO,.5H,O and cb that of CuCl, . 2H,0. 

d. The system CuCl,— KCl — H,O. 

In this system of which the invariant (P) equilibria were 

1) P. A. MeerpurG. Gedenkboek J. M. vAN BEMMELEN, 356 (1910). 

2) BRuNNER. Pogg. Ann. 15 476 (1829). 

3) F. A. H. ScHREINEMAKERS. These Communications l.c. and Zeilschr. Phys. Chem. 
69 557 (1909). 


5385 
examined’ formerly ') oceur as solid phases: KCl, CuCl, . 2H,0, 
CuCl, . 2KCl.2H,0 and CuCl, . KCl. This last salt, however, occurs 
only above 57°, so that, at 30°: KCl,CuCl,.2H,O and CuCl,. 
2KCl.2H,O only occur as solid phases. 

The isotherm of 30° is represented schematically in fig. 1; fe is 
the saturationcurve of KCI, cd that of CuCl, .2H,O and ed that of 
CuCl, .2KCl.2H,O. When we represent in fig. 1 this doublesalt by 
D,.,.,, then the line WD,.,., does not intersect curve ed, but curve fe. 
This doublesalt is, therefore, at 30° not soluble in water without 
decomposition, but it is decomposed with separation of KCl. 

This isotherm of 30° was determined already formerly *); we 
have also still determined some points. 


3. The quaternary system. 


At first sight we may think that the examined system is built 
up by five components; as, however, between four of these substances, 
the reaction : 

Cul, > Ke SOp a KCl CusOes = 2  D 
oecurs, this is not the case. 

In view of the above-mentioned double-decomposition (1) we shall 
represent the equilibria with the aid of a quadrilateral pyramid, the 
base of which is a quadrangle. The four anglepoints of this qua- 
drangle indicate the four substances: CuSO,, CuCl,, K,SO, and K,Cl, 
and in this way that the two substances, which are in reaction (1) 
at the same side of the reaction-sign, are united by a diagonal of 
the quadrangle. Perpendicular above the point of intersection W_ of 
the diagonals, is situated the top of the pyramid, which represents 
the water. 

At the examination of this quaternary system we have always 
remained below the temperature, at which the basical salt 

4Cu0. K,O. 450,. 3H,0 
is separated. If this had not been the case, the reaction : 
4CuSO, + K, S50, + 4H,0 2 4Cu0. K,0. 480,. 3H,0 + H,SO,. (2) 
would have occurred. We should then have had to examine a 
quinary system, in which reactions (1) and (2) occur. 

As the quaternary solutions saturated with a solid substance, are 
represented by a surface in the space, viz. the saturationsurface, we 
have seven saturationsurfaces. We find their projections in fig. 1 ; 


1) W. Meyeruorrer. Zeilschrift fiir Phys- Chem. 0 336 (1889) 5 97 (1890). 
2) H. Frutppo; not yet published. 


536 


from this it is apparent that six of these surfaces are side-surfaces 
and that one is a middle-surface. 


aklm6 is the saturationsurface of the CuSO,. 5H,0 


ClO eee > 5 CU CIE ALG 

adnoe. ae i 5 on POW). 2KCII2AE® 
eopg ie AH ace 50 2 KCl 

GG Cl es 4 Sy Ke SO, 

iqlk » £ Re op OW SO KE ISO) .(Blal-(O, 
pqlimno,, 5, 3 Rae es 58) 


In order to get a better view, in the figure is indicated on each satura- 
tionsurface the solid substance, with which the solutions are saturated. 
For the sake of abbreviation we bave called Cu SO,. 5H,0 = Cu,, 
Cu Cl,. 2H,0 = Cu,, Ca Ch. 2KCI. 2H;0 = D..,., and CuSO; Kes@2 
GHEO Dg : 

The middle-surface pq /mo is the saturationsurface of a salt, which 
we have represented by J. In order to find the composition of this 
salt we have applied the rest-method, viz. the analysis of the solution 
and the corresponding rest. From numerous definitions it follows 
that this salt has the composition : 


CwsO Kk Ce Ke son CalCit— Ds 
or CuSO,. K; Cl, 8,0 =K,S0,1Ca Cle HO ae 


Some determinations pointed viz. to D,, others to Dx, again others 
to a mixture of D, and Dx, so that in the region pqim no (tig. 1) 
perhaps the two salts D, and Dx occur. 

The probability that more than one solid salt occurs in this region, 
is enhanced by the following observations. In some eases the solid 
substance was precipitated after shaking (which lasted sometimes a 
month or longer) within some hours as a greenish powder, in other 
cases there was formed a greenish or blue-greenish paste, which 
after days did not yet settle, but stuek to the sides of the shake- 
bottle. In the first case we could easily remove a large part of the 
mother-substance by suction, in the latter case this appeared practi- 
cally impossible. From all this it is. apparent that in the saturation- 
surface (fig. 1) indicated by D different salts may occur, two of which 
have the composition D, and Dx. 

[t follows, however, from the position of the solutions saturated 
with D, or Dx in the region of fig. 1 indicated by D, that one of 
these salis must be metastable with respect to the other, perhaps 
they are both metastable with respect to a third, which we have 
however not found in onr investigation. 


537 


In order to get the solutions of the saturationsurface D saturated 
with solid salt, we put together the substances in such ratios 
that the solid substance must be formed in one case from 
Cu SO, .5H,O + KCl, in the other from Cu Cl,. 2H,0 + K, 50,. In 
both instances now D, then Dx was formed. 

In some cases also occurred as solid phase a double salt of the 
composition : 

2Cu SO,. 3K, Cl,. H,0 =D, 
Later, however, we did not succeed again in getting this salt, but D, or 
Dx, appeared instead. The salt D, will therefore, very probably exist 
in a metastable condition only. 

On account of the uncertainty with respect to the substance D, 
we will further describe the equilibria as if in the region p q/in no 
occurs only one solid substance D. When in this region more solid 
phases may occur in stable condition, then the necessary changes in 
this region will have to be inserted. 

The intersectinglines of the saturationsurfaces represent the quater- 
nary solutions, which are saturated with two solid substances, con- 
sequently the quaternary saturationlines. The limit-lines of the 
saturationsurfaces on the side-planes of the pyramid form the ternary 
saturationcurves of the four ternary systems, which have already 
been discussed previously. 

The quaternary saturationcurves are the following : 


gp the saturationline of K, SO, + KCI 


COR ss a 9 it, SO, ce Dyas, 
eles paous » Sa Dic. 
bm ,5 3 » Cu, + Cu, 
dn the saturationline of Cu, + D,.,., 
BIO) os i iy KOh = Ding 
OU + +5 5 K,SO,4+ D 

Gl ne ‘5 5 D4 
ieee is 7 Cle 
oe 3 » Cuy +D 
WiOw 5 x oe Diet sD 
OP os be + ACE tp 


The first six saturationlines are side-curves; each of these has an 
end on one of the side-planes of the pyramid. The last six satura- 
tionlines are middle-curves; each of these has its two ends within 
the pyramid. 


538 


The points of intersection of the saturationsurfaces represent the 
quaternary solutions, which are saturated with three solid substances 
consequently the quaternary saturationpoints. In each of these points 
three quaternary saturationcurves come together. In the ternary 
saturationpoints, which we already discussed previously, two ternary 
and one quaternary saturationcurve come together. 

The quaternary saturationpoints are the following: 


p saturated with K,SO,-+ KCl + D 


q - » K,SO,+D,.,..> D 
l 7 » Cu, © = Dew dD 
m 3 3. (Cu; ) =eiCiss ap 
n 5 5 Olu. + D,.,., + D 
Onan ICH SE Ds 25 1D 


As it is easy to see from fig. 1, in presence of solution can exist: | 
K, SO, by the side of: KCl or Dor D,.,., 
but not by the side of: Cu, or Cu, or D 
KCl by the side of: K, SO, or D or D,.,.,. 
but not by the side of: D,.,., or Cu, or Cu, 
ig-, Dy the side of: KCl or D or Cu, 
but not by the side of: K,SO, or D,.,., or Cu,. 
Cu, by the side of: Cu, or D or D,.., 
but not by the side of: KCl or K, SO, or D 
Cu, by the side of: Cu; or Dior D;.., 
but not by the side of: K, SO, or KCI or D 
D,.,., by the side of: Cu, or D or K,SO, 
but not by the side of: KCl or D,.,., or Cu, 
D by the side of all other substances. 


HOE Wy | 


D 


TSS 


12353 


Different conclusions can be made from the figure. Let us con- 
sider the behaviour of the salt D with respect to water. 

When D is the salt D,, it is indicated in the spacial represent- 
ation by the point of intersection W of the diagonals (fig. 1). When, 
however, D is the salt Dx, which contains water, it is situated in 
the spacial representation on the line, which unites the top of the 
pyramid with the point of intersection of the diagonals. Let us 
assume that D—=D,z and let us call T the top of the pyramid, so 
that point T represents the water. As the line D,T does not inter- 
sect the saturation-surface of D,, Da is not soluble in water without 
decomposition. The line D,T intersects, however, the saturation- 
surface zklq of D,.,.,, so that the salt D, = Cu'SO,. K, Cl, = K, SO,. 
Cu Cl, is decomposed by water, while D,.,., = Cu SO,. K, SO,.6H,O 
is separated. From this we see that we can not wash out the salt 


539 


D, with water to free it from its mother-substance, as this will 
lead to decomposition. 

When we wish to examine accurately what will take place when 
we bring together D, and water, we must consider which spaces 
of the pyramid are intersected by the line D,T. From this amongst 
others the following is apparent. When we add D, to water, then 
firstly unsaturated solutions arise, which are represented in fig. 1 
by the point W. (In this it is to be considered that fig. 1 is the 
projection of the spacial representation and that point W is the 
projection of the line D,T). , 

With further addition of D, the solution W arises, which can be 
saturated with D,.,., (this D,.,.,. however, is not yet present as 
solid phase) consequently the solution W of the saturationsurface zq//-. 

With further addition of Dz now D,.,., is separated and the 
solution traces in fig. 1 the straight line Ws, this straight line is the 
projection of a curve situated on the saturationsurface 7q/k. When 
we add so much D, that the solution attains the point s, then, 
further addition of D, will no more change the solution and there 
is formed: 

D,.,., + Da + solution s. 


When we wish to examine what will take place when we bring 
together in variable quantities K,SO0,,CuCl, and water, then we must 
intersect the spacial representation by the plane K,5O,—CuCl,—T. 
When we bring together KCl— CuSO, and water in variable 
quantities we must draw the plane K, Cl, — CuSO, — T. 

As the manner, in which these sections with the saturationsurfaces, 
saturationlines and the different spaces can be obtained, was already 
discussed previously *), we will not apply this method now. 

In tables If and III we find indicated the compositions of several 
solutions; we have deduced with the aid of the restmethod graphically 
the solid phases with which these solutions are saturated. 

In table II the compositions are expressed in percentages by weight ; 
of the four salts Cu SO,,Cu Cl,, K,SO, and K, Ci,; only three at the 
same time are given. This is sufficient also because, if we wish to 
express the composition also in the fourth salt, it may be done in 
infinitely many ways with the aid of the reaction-equation 

Cu SO, + K, Cl, 2 K, SO, + Cu Cl, 

For this the quantities of the substances which take part in the 

reaction must be expressed in quantities by weight. 


1) k. A. H. Scoremnemakers. Zeitschr. f. Phys. Chem. 66 699 (1909). 


540 


ACE ese. 
The ternary system K, SO, — KCl — H2O at 30°. 


Composition of the solutions 


in proc. by weight | in molproc. 
| 


Point Sie Solid phase. 
K,SO, | KCl H20 | K,SO4 | KeCh | H,0 


epee 0. Wests i a-33 0 | 98.67 K»SO, 
2.55 | 17.45 | 80.0 | 0.32 | 2.56 | 97.12 


” 


ge |e 4209.) 26.20.) 72.7. |, OMS: |) 4516 *) $95.69 K,SO, + KCl 
oe 0 222. 72.78 Oi 432 95.68 KCl. 
ABLE Il 
The quaternary system Cu SO, — Cu Cl, — Kz SO, — K,Clz — H20 at 302. 


Composition of the solutions in procents by weight. 


Point CuSO, | CuCl, | Kp SO, | KCl 
K | 20.60 On ali 3%61 0 | 75.79 | Cie ee 
14.60 5 23a seus 0 76.44 | . 
Ex | 10.02 | 10.74 | 4.56 0 | 74.68 | i 
7 1.70 | 24.48 | 6.92 0 | 66.90 | i 
1 | 7.43 | 23.75 | “0 6.26 | 62.56 | Cue Dig gen 
i 1.63 0. | 12.01 | 0 | 65.36.| | Kiso -=DRe 
1.63 oll ave | 2.98 | 86.26 A 
1.2] 0 6.76 | 6.01 | 85.51 7 
Es | o | 213 | 5.74 | 9.84 | 82.29 : 
% 0 5.05 | 3.82) |) Gl6s02) |) 75.11 . 
2.96 | 6.07 | o | at.e6 | 69.11 . 
q 2.97 | 6.68 0 | 21.97 | 68.38 | K,SO4+-Dj..6--D 
g 0 o | 1.09 | 26.20 | 72.71 | kj S0,4+KC 
ae | 1.75 4.80 | 0 | 25.32 | 68.13 5 
“>. [acest “6-86 | 24.68 | 66.70 | Ky SO,-+ KCl-+ D 


| | 


541 


TABLE Ir 
The quaternary system: Cu SO,— Cu Clz — K, SO4 — KoCl, — H,,0 at 30°. 


Composition of the solutions in procents by weight. 


Point | CuSO, | Cu Cl. | Ky SO, | K Cl | H,0 | Solid phase. 
p 2.06 | 6.56 | 0 24.68 | 66.70 | k_)SO,+KC1-+D 
g_ | 234 | 61 | 0 23.32 | 67.60 | K,S0,-+D 
Girl) /2-6f || "63 |. <0 22.17 | 68.59 | r 
q | 2.97 | 6.68 | 0 21.97 | 68.38 KSOn= Dire eD 
q 2.97 | 6.68 | 0 21.97 | 68.38 KeSOreEDaeeD 
2.04 | 7.86 | 0 17.03 | 68.92 Be 
[esate 111.00 On Slt. ste set - 
Ee | 4:08 | 17.31 0 | 11.81 | 66.79 re 
= || vaces | 20:80 0 9.44 | 65.41 7 
| 7.53 | 23.31 0 6.63 | 62.53 | : 
l 7.43 | 23.75 oO Weeo5 loose | Cue Die ED 
p | 2.06 | 6.56 0 24.68 | 66.70 KeSO0, = KID 
| i.54 | 9.22 0 23.64 | 65.60 KCI-+-D 
| 1.34 10.86 0 93.11 | 64.69 i 
g | 1.30 | 11.29 =O 22.80 64.11 
S™ | 0.80 | 16.95 0 21.28 | 60.97 | i 
0.75 | 17.51 | 0 | 21.35 | 60.39 | 2 
0.72 | 18.56 0 21.37 | 59.35 
0 0.56 | 21.43 | 0 | 20.47 | 57.54 KiCHED Dim 
| | 
Sar: 21.62 | 0 | 20.86 | 57.52 Keele oD pss 
o 0.56 | 21.43 er | 20.47 | 57.54 | KCl+D+Dh.2 
| | 
oo O-scre| 21.48 0 20.47 | 57.54 | KCIED+Dio0 
| 0.59 | 26.09 0 16.83 | 56.49 | Dee Diss 
a 0.63 | 29.41 | 0 | 15.01 | 54.95 | ' 
S | 0.71 | 32.60 0 13.10 | 53.59 r 
0.70 | 37.61 0 10.62 | 51.07 | , 
n 0.4 | 424 | o | 7.86 | 48.75 | €u+-D+Dio 


| | | | 


TABLE Il 
The quaternary system: Cu SOy— Cu Cl) — Ky SOs — Ky Cl, — HO at 30°. 


SS 


Composition of the solutions in procents by weight. 


Point | Cu SO, | CuCl, | K,SO, | KCI H,O | Solid phase. 
n 0.94 | 42.45 0 | 7.86 | 48.75 Cu, +D +Dj29 
™ | 
d 0 | 43.1 ou 84 48.5 | Ci, Dien 
n 0.94 | 42.45 | 0 | 7.86 | 48.75 Cu, De apeee 
zs | “1.59 | 42.30 | 0 4) 52884] 50Ke3 Cu, -+D 
oe $.46.1\ 40.95 0s 0). lee anade | ates Cu; “Gus aR) 
| | 
m 3.46 | 40.95 | 0 | 4.34 | 51.25 | Cu, 42 Cu; D 
b Deal LOR Ou) | SOU mlunstes4 Cu, + Cus 
3.46 | 40.95 | 0 | 24.34 | {51225 Cus ens 
, 4.15 | 36.69 | 0 4.79 | 54.37 Cuca 
ae | 4.48 | 34.33 0 | 5.14 | 56.05 . 
= 5.48 | 29.55 0 5.74 | 59.23 
Phe) eas | 23.75 0 6.26 | 62.56 Cus 4 Dia 
| 4.90 | 24.49 0 7.64 | 62.97 
| 2.88 | 10.71 0 18.57 | 67.84 
2.29 | 10.44 0 90.12 | 73.15 
2.15 | 10.83 | 0 19.97 | 67.05 | 
: outs | Giles 0 19.60 | 65.89 
. teoeelp Cli be 21.24 | 66.00 
E 1-31 4/16 267. lg ane 18.54 | 63.48 
E 1.31 | 16.57 | 0 18.68 | 63.44 
e 0.89 | 23.19 0 16.38 | 59.54 
A 854 |e23.15° 4/10 16.25 | 59.17 
0.669 |) =2160i-aO 15.92 | 61.62 
|) 91:03 | ie2me0 0 13.70 | 58.17 
| oc | 32.57 0 12.43 | 54.23 | 
| 2.03 | 27.75 | a) 9.93 | 60.29 | 
| 4.47 | 39.14 0 7.17 | 52.25 
| 
6.06 | 19.84 | 0 7.75 66.35 | Saturation surface Dj.;.g 
\ i 


543 


TA BIE, Ul 


The quaternary system: Cu SO4— Cu Cl, — Ky SO, — Ky Cl, — H; O at 30°. 
Ions Cu, Ky, SO, and Cl, and Mol. H,O in a quantity of 
solution which contains 100 Mol. in all. 


Point Cu K, SOF) Cl; H,O | Solid phase. 
| 
K 2.96 | 0.48 | 3.44 | 6 96.56 . Gis -eDire 
2.97 | 0.49 | 2.51 | 0.89 | 96.54 | i 
a 3.34 | 0.61 2.10 1.85 | 96.05 $ 
: 4.88 1.01 1.28 | 4.61 | 94.11 . 
l 5.98 112 1.25 | 5.85 | 92.90 Gust Dia oD 
oe A So DS 
i Oe | er ace 0 Ognash ly | a KaSOh Dit 
0.21 1.49 1.29 | 0.41 | 98.30 ‘ 
0.22 1.64 1.03 | 0.83 | 98.14 é 
Ex 0.34 Dai GE70) lee Te toe |cO7-55 > 
> 0.86 | 2.98 | 0.51 3.33 | 96.16 < 
1.58 | 3.62 | 0.46 | 4.74 | 94.80 ¢ 
q 1.70 | 3.68 | 0.46 | 4.92 | 94.62 Ke SO; oD 
ig Oh Te) 4-31 Pros 15) |b 4516)" | 95.69 K SO,-+ K Cl 
58 1.17 | 4.25 | 0.28 | 5.14 | 94.58 | p 
. 1.56 | 4.21 0.33 | 5.44 | 94.23 K, SO,-+K Cl+D 
p 1.56 | 4.21 0.33 | 5.44 | 94.23 K,SO,+KCl+D 
wi 1.63 3.94 | 0.37 | 5.20 | 94.43 | K,SOn-D 
Sie 1.64 | 3.70 | 0.41 | 4.93 | 94.66 | i 
q 1.70 | 3.68 | 0.46 | 4.92 | 94.62 | K,S0y+-D+4 Dis 
q (710i? 3.68 a fe O:46.4|-4 14.92 \)eod G2 Lh KG SO," DAL Dit, 
1.92 3.51 | 0.46 4.97 94.57 DitesaD 
2.52 2.89 0.49 | 4.92 | 94.59 A 
aa 3.92 2501s.) 0.64 |- | (5.29 94.07 . 
= 4.68 1.63 | 0.78 | 5.53 | 93.69 r 
5.90°| 1.19 | 1.26 | 5.83.| 92.91 ‘ 
l 5.98 1.12 | 1.25 | 5.85 | 92.90 Gite Dates D 


kK 


544 


TABLE Ill. 


The quaternary system: Cu SO,— Cu Clp — Kz SOy — K, Cl, — H, O at 30°. 
Ions Cu, Kg SO, and Cl, and Mol. H;O in a quantity of 


solution which contains 100 Mol. in all. 


Point Cu kK, SO, Cl, HO Solid phase. 
p 1.56 | 4.21 | 0.93 | 5.44 | 94.23 K, SO4-+-KCI-+D 
2.02 MF acs | 0.25 | 5.85 | 93.89 KCI--ED 
2.33 | 4.04 | 0.22 | 6.15 | 93.63 a 
a 2.40 | 3.99 | 0.21 6.18 | 93.61 - 
S™ | 3.58 | 3.90 | o14 | 7.98 | 92.92 2 
3.72 |.3.95 )|2 0.18 | 7.54 1) 92.33 
3.98:| 4.00 | 0.12 | 7.86 | 92.02 55 
o 4.66 | 3.93 | 0.10 | 8.49 | 91.41 K Cl-E D+ Dies 
e 4.58 | 3.93 | o | ssi | 149 KGEsDies 
0 4.66 | 3.93 | 0.10 | 8.49 | 91.41 K Cla= Dis ee D 
o 4.66 | 3.93 | 0.10 | 8.49 | 91.41 K Cl DyaaeeD 
5.74 | 3.27 | 0.11 | 8.90 | 90.99 DaeDies 
2 6.60 | 2.98 | 0.12 | 9.46 | 90.42 . 
Or 7.46 | 2.66 | 0.13 | 9.99 | 89.88 f 
8.91 2.23 | 0.14 | 11.00 | 88.86 Z 
n 10.44 1.71 0.19 | 11.96 | 87.85 Cu Dag 
n 10.44 | 1.71 0.19 | 11.96 | 87.85 Ci; 4D sa 50 
d 10.44 | 1.84 0 | 12.28 | 87.72 Cug- Diss 
n 10.44 | eel 0.19 | 11.96 | 87.85 Cig Dj oa 
as 10.30 | 1.25 0.32 | 11.23 | 88.45 Cu, + D 
Su eao.19, ora 0.68 | 10.42 | 88.90 Cu,+Cu; + D 
m 10.19 0.91 | 0.68 | 10.42 | 88.90 Ca, Gin 
b 10.03 | 0 0.54 | 9.49 89.97 Cu, + Cus 


545 


TABLE Ill. 
The quaternary system: Cu SO4— Cu Cl, — K, SO, — K, Cl, — Hy O at 30°. 
Ions Cu, K, SO, and Cl, and Mol. H, O in a quantity of 
solution which contains 100 Mol. in all. 


Poittty ee Cua) KG | SO, ch | H,O Solid phase. 
| " | 
: 
m 10.19 0.91 | 0.68 | 10.42 | 88.90 Guy |: Cu, 4 D 
8.93 | 0.94 | 0.78 | 9.09 | 90.13 Cup-+D 
8.27 1.01 | 0.82 | 8.46 | 90.72 | fr 
| 
7.10 1.07 | 0.96 7.21 | 91.83 | é 
l 5.98 1612 | 1.25 5.85 | 92.90 |  Cus-++Dy1.6-+D 
| 5.67 1.36 | 0.82 21 | 92.97 


2.38 | 3.39 | 0.34 43 | 94.23 
2.49 | 3.34 | 0.34 49 | 94.17 

A 2.38 | 3.65 | 0.28 75 | 93.97 | 

2 3.50 | 3.29 | 0.22 | 6.57 | 93.21 

i 3.48 | 3.32 | 0.22 | 6.58 | 93.20 

2 4.96 | 3.06 | 0.16 | 7:86 | 91.98 

3 5.09 3.05 0.15 7.99 | 91.86 


4.73 less | 0.97 5.09 93.94 Saturation surface Dy.;.¢. 


In table III the compositions are indicated in the number of ions 
Cu, K,, SO, and Cl, and molecules H,O, which are present in a 
quantity of solution, which contains in all 100 molecules. 

When a solution contains a ions Cu, 4 ions K,, c ions SO,, d ions Cl, 
and w molecules of water, then is consequently 


atb=c+d-ndwt+a+t+b=w+ce+d=100. 
Leiden. Anorg. Lab. Chem. 


546 


Chemistry. — “The catalyse”. By Prof. J. Bousexen. (Communi- 
cated by Prof. A. F. HoLieman). 


(Communicated in the meeting of June 27, 1914). 


1. It appears to me that, a summary having been given from 
various quarters on catalytic phenomena, the time has arrived to 
show briefly how the development of my ideas on this subject has 
advanced and how the insight thus gained has been supported by a 
deduction of one of my students. 

I do this in the first place because in that historical account the 
eradual elucidation of the phenomena is exposed, but also because 
I imagine that a point has now been reached where the co-operation 
of many is necessary in order to assist in completing the edifice of 
the catalysis. 

2. When working at my dissertation (1895—1897), when a large 
number of fatty-aromatic ketones was prepared according to the 
reaction of Frinper and Crarts, it struck me that when to a cooled 
mixture of acid chloride and benzene finely powdered aluminium 
chloride was added, this certainly dissolved rapidly, but that an 
evolution of hydrogen chloride only took place slowly on warming’). 

As aluminium chloride did not perceptibly dissolve in benzene, 
I was then convinced that not the benzene but the acid chloride 
might be the point of attack of the catalyst. 

This question was afterwards taken up by me and solved in so 
far that the synthesis of the aromatic ketones could be divided into 
two stages: (a) The catalyst combines with the acid chloride: (b) 
this compound is attacked by the aromatic hydrocarbon (Rec. 19 
19 (1900) 20 102 (1901). 

Although the course of the reaction was indicated therewith, I 
was soon aware, however, that the catalytic action of aluminium 
chloride remained in complete obscurity *). 

In this I was corroborated by the observation that chloroform 
and benzyl chloride suffered the reaction with benzene still far 
better and more vigorously, whilst these substances did not combine 


1) Afterwards | modified the preparation by taking the AICls in excess and then 
adding drop by drop the mixture of acid chloride and benzene, because the reaction 
then proceeded very regularly. By the research of OLIviER (Dissertation, Delft 1912) 
it has been shown that the cause of this favourable result must be attributed to 
the presence of free AIClg (see later). 

2) PERRIER who had noticed this reaction course previously (Thése, Caen 1893) 
was of opinion that this explained the catalylic action of aluminium chloride. 


547 
with aluminium chloride and the quantities of the catalyst necessary 
for the reaction were much less than in the synthesis of the ketones. 
(Ree. 22, 301 (1903)). 

When it appeared that nitrobenzyl chloride, which does unite with 
AICI,, was also attacked much less rapidly than benzyl chloride, 
and further that the very reactive anisol, which also forms a molecular 
compound with AICI,, 
did so readily, the facts were such that | ventured the thesis that 
the formation of compounds between the catalyst and the activated 


did not react ad a// with CCl,, whereas benzene 


substance had nothing to do with the actual catalytic action (Ree. 
23,104 (1904)) and that, when the catalyst does not unite with one 
of the substances present in the reaction, we are dealing with catalytic 
action in its purest form (Rec. 24, 10 (1905)). 

Thus by means of the inductive method, | came to the conclusion 
that the formation of a compound with the catalyst did not give an 
explanation of the catalytic action as such, and that with this the 
theory of the intermediate products exploded. 


2. I have also tried to demonstrate subsequently by means of the 
deductive method that the formation of a compound of substance and 
catalyst must necessarily lead to a partial paralysis of the latter 
(Proc. 1907 p. 613; 1909 p. 418). 

Hence, if we wished to arrive at a satisfactory explanation this 
had to be looked for in what happened before there is any question 
of a compound between catalyst and substance. When the catalyst 
draws near to the activated substance a phenomenon ought to take 
place partaking more of a disruption or a dislocation than of a union 
(Gedenkboek vAN BeMMELEN p. 386, Rec. 29, 87 (1910)),. 

I have then demonstrated (Proc. 1909 p. 419; also Rec. 32, 1 
(1913); Chem. Weekbl. 7, 121 (1910); Rec. 29, 86 (1910)) that a 
catalyst like AICi, exerts indeed a dissociating influence on the 
chlorides which it activates; chloral was resolved into CO, HCl and 
©,Cl,;  trimethylacethyl chloride into carbon-monoxide, HCl, and 
isobutene, ete. 

But here it transpired also that even now the explanation was 
not given, because the action had been too violent; instead of the 
to be expected condensation products with benzene there were 
obtained in similar cases, either the decomposition products or the 
condensation products of these molecule residues with benzene. Thus, 
from SO,Cl, and the benzene hydrocarbons were generated relatively 
very small quantities of sulphones compared to large quantities of 
sulphinie acid and chlorine derivatives; owing to too great an aciivily 

36 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


548 


the catalyst had disrupted the SO,Cl, into SO, and Cl, which were 
now subsequently influenced catalytically (Rec. 30, 381 (1911)). 

The catalytic action proper can, therefore, be no union, because 
in that compound the catalyst is paralysed; it also cannot be a 
dissociation because the substance is then too much attacked, hence, 
it must be an intermediary influence. 

I have called the latter a dislocation or disruption (Ree 80, 88 
(1911) dating from Sept. 1909) in order to demonstrate that there 
certainly does exist an influence, but that this should effeet neither 
union or dissoeiation if it is to be considered as a purely catalytic 
one. In order to more sharply confirm experimentally this result 
obtained, the transformation of chloral into metachloral under the 
influence of diverse catalysts was submitted to a closer investigation. *) 

This system was chosen because it had been shown that: 

1st it is an equilibrium between two substances, therefore a very 
simple ease because we are only dealing with the transformation of 
one substance into another one. 

2nd this equilibrium is situated in a readily attainable temperature- 
zone, whereas the properties of monomeride and polymeride differ 
rather strongly, so that the specific influence of the catalyst may 
come perceptibly to the fore. 

394 That the monomeride itself is a supercharged molecule, so 
that it was to be expected that the action of the catalyst would be 
a pronounced one. 

In fact it could now be demonstrated that the equilibrium 
was attained rapidly only then when the activator was present in 
small quantities and had not perceptibly united with one of the 
modifications. 

If the catalyst (pyridine) was retained (absorbed) in the colloidal 
polymeride the equilibrium set in, but in the hquid phase of the 
monomeride the reaction ceased. 

If the catalyst combined with one of the components (the mono- 
meride) the equilibrium was shifted in the direction of that component. 

If, finally, the action of the activator was stronger still, the split- 
ting products were obtained only. 

About the same time, S. C. J. Outvier (Diss. Delft 1913, Proe. 
1912 and R 88, 91 (1914) had finished a dynamic research on the 
action of bromobenzenesulphochloride on some benzene-hydrocarbons 
under the influence of aluininium chloride. 

Whereas the researches had been as yet of a qualitative character 
it could now also be demonstrated quantitatively that the retention 


1) KR 32, 112 (1913). 


549 


of the eatalyst in the sulpho-chloride or in the sulphone caused a 
partial paralysis, as the reaction proceeded much more rapidly the 
moment a small quantity of the catalyst in the solution was present 
in the free state. 

Also, could it be deduced sharply from the progress of the reaction 
(Proe. 1913 p. 1069) that this could be explained satisfactorily only 
then when the activating action was sought in) what happened 
between benzene on one side and chloride + catalyst on the other 
side before they had undergone chemical transformation. 

Hence, it was proved experimentally also here that the most important 
stage of the catalysis is that which takes place before the union. 


3. If we now consider what can be the significance of the 
removal of the catalysis to the pre-stage of the reaction, it should 
be remembered that in view of Ostwatop’s definition a catalyst should 
be a substance unchanged in quantity and quality after the reaction. 

Guided by this definition we may during the reaction assume all 
kinds of material and energetic changes if only the condition is 
satisfied that the catalyst remains unmodified before the beginning 
and after the end of the reaction. 

If now, however, we look for a further explanation, that is to 
say, penetrate further into the mechanism of a reaction, we notice 
that somewhere during the reaction a catalyst can no longer satisfy 
that definition. 

Hence, a catalyst can never remain unchanged during the entire 
course of the reaction; an ideal catalyst exists no more than an 
ideal gas or an ideal dilute solution, but for all that we have been 
able to make excellent use of the notion. 

Now, a substance will approach this ideal condition all the more, 
the smaller the material or energetic displacements will be and it 
is plain without any further evidence, that similar very small changes 
will just take place on the approach of the catalyst to the bonds to 
be activated. 

When there the action ceases, we can understand that these 
shiftings may be so small that they elude observation (so that for 
instance, apparently a same equilibrium is reached under the influence 
of diverse catalysts, which in reality cannot be the case.) 


4. If now we want to get a concrete conception of these exceed- 
ingly small actions, which in the catalysis are both satisfactory and 
authoritative, we may consult the modern views on our atomic. 
world. 


36 


550 


It is supposed that the atoms consist of (or at least are populated 
by) electrons and that they hold together by means of force regions 
between these corpuscles; the catalytic action may then be deseribed 
as a change of these force regions on the approach of the catalyst. 
If this is so, we have in the pure photocatalysis the simplest 
catalytic actions and the study of these phenomena will no doubt 
much deepen our insights. *) 

On penetrating further into the phenomena in general we are 
obliged to resolve the substance into steadily decreasing units and 
the same has happened with the special phenomena called catalytic; 
here it will just be shown that what takes place in the atoms will 
be of preponderating importance. But just as we have not been able 
to find the ideal catalyst among the atoms, we cannot expect to 
meet it among the electro-magnetic equilibria-perturbations, only 
the limit of our insight in the catalytic phenomena has advanced 
a step. 


Il. 


1. During this mainiy inductive development of my ideas my 
pupil H. J. Prtxs had found a synthesis of chloropropane derivatives 
and I advised him to couple this experimental subject with a survey 
of the different cases in the reaction of FrispeL and Crarts. *) 

With this, however, he did not content himself, but starting from 
the “Principle of Reciprocity” he has endeavoured to furnish an 
explanation of the catalytic phenomena in general, with the reaction 
of Friepet and Crarrs as a special case. 

The result of this is given in his dissertation (“Bijdrage tot de 
kennis der katalyse’, Delft 1912) and supplemented with a few 
subsequent articles (Journ. f. pr. Chem. N. F. 89, 425 (1914); 
Chem. Weekbl. 11, 474 (1914). 

In order to reproduce Prins’s intention in the simplest possible 
manner, | will quote a few parts of his deduction, taking the liberty 
to omit the, in my opinion, non-essential matter. 

1) The simplest case is the photocatalytic change of a monatomic element. 

2) The reaction of FR. and Cr. offers us already a great diversity of catalytic 
reactions, because AICI; can form all kinds of compounds. Only in such cases 
where it unites neither with the initial products nor with the end product, or attacks 
this secondarily do we approach a case ef pure catalysis. 

The number of these cases is very small, the chlorination of benzene is a very 
appropriate example thereof; here the quantity of the catalyst is minimal indeed 
(see further) 


The axioms which are more particularly applicable to the cata- 
lysis are: 

“When... the one exerts an influence on the other, this latter... 
is changed by the first... 

“If in the calculation of one of these the change may be neglected 
we may speak of a one-sided influencing, which, however, as such... 
may not be considered one-sidedly (dissertation p. 4—5). 

and subsequently : 

“If we consider the possible relation of two substances (whether 
element or compound) three stages are to be distinguished therein’. 

“J. The stage of the relative inertness. In this stadium even 
the catalytic influence is imperceptible, whilst there is no question 
of a chemical compound. 

“2. The catalytic stage’) in which occurs also the mutual acti- 
vation. In this stage the catalytic actions are enacted. 

“3. The reaction stage in which appears an intra- or extra- 
molecular reaction”. 

The catalytic stage forms the bridge between the inertness and 
the chemical compound. In each chemical reaction all three stages 
are gone through. 

By varying the conditions we can, however, cause the influencing 
to be confined to the second stage’. (Chem. Weekbl. 11, 475, 
also Journ. f. pr. Chem. N. F. 89, 448 (1913). 


2. Prins starts from the general thesis that on interaction, there 
takes place a change in two conditions, which will be least powerful 
the moment it begins to reveal itself. 

This stage lies, chemically speaking, in the dissociation region 
where the free energy of the entire system approaches to zero 
and is called by Prins the catalytic stage. 

In this catalytic stage there is really no question of a catalyst 
in the sense of OstwaLp; we are dealing with a change of condition : 
AZB which taken by itself can take place more or less rapidly. 

Being in the catalytic stage does not at all imply, in my opinion, that the 
changes must take place rapidly; this depends on the nature of the change 
(chemically speaking on the nature of the atoms or atomic groups which in the 
transformation play a role in the first place). 

If, for convenience sake, we call A and B two molecules. one 
of these molecules, in a reaction in which the other one (with its 


1) In order to prevent confusion it would be better to speak of the activating 
stage. (PRINS also points out that the word “activator”? expresses his ideas better 
than catalyst). 


552 


specific atomic group) occurs as a component, will be a catalyst 
in the sense of OsTWALp. 


BSC A—>D 


N N 
A B 


The above symbols represent this explanation from which we gather 
that the change of the’free energy in so far as it concerns the catalyst 
approaches in the pure catalysis to zero and wherewith we also wish 
to express that the catalyst is in faet more a change of condition 
than a substance. , 

In the positive catalytic action the equilibrinm A <> Bb will set in 
much more rapidly than the reaction B—+C or A—D and thus 
cause or accelerate the same. 

Hence an ideal catalyst, according to this deduction and in connexion with 
OstwWatp’s definition, is a substance which undergoes with one of the to be 
activated substances (or bonds) such reciprocal action that in the latter 


system the thermodynamic potential and chemical resistance simultaneously 
approach to zero. 


As it concerns here particularly the bond that is being activated, 
the other moleeule wili also be more or less influenced; this we 
notice immediately when we remember that intramolecular displace- 
ments come under the same point of view. 

Hence, we will obtaim the maximal catalytic action when, with 
the catalyst (for instance Bb) we approach as closely as possible the 
catalytic stage in regard to A as well as D. 

The chlorination of benzene again presents us with a suitable 
meaning example to elucidate the intention of this thesis. 

Both chlorine and benzene are in regard to AICI, in the catalytic 
stage; they are both rendered active without forming a compound. 

As soon as we replace benzene by nitrobenzene the action ceases 
at the ordinary temperature because A/C/, forms a solid combination 
with nitrobenzene so that these two are, in regard to each other, 
not in the catalytic stage and because AICI, cannot any longer 
activate the chlorine simultaneously. 

At a higher temperature the chlorination starts; we may assume 
that the system A/C7,NO,C,H, is then again approaching the 
catalytic stage. 

It is, however, self-evident that a case like the chlorination of 
benzene is rarely met with; as presumably somewhat similar cases 
I mention: all ionreactions in aqueous solutions; the union of 
hydrogen and oxygen and the decomposition of hydrogen peroxide 


on or in platinum; the transformation: aldehyde = paraldehyde 
under the influence of sulphuric acid ete. 

Much more frequent will be the cases. such as in the chlorination 
of nitrobenzene, where the catalyst is found, in regard to one of 
the substances, a good long way over this most favourable stage ; 
in that case it will have united with one of the components to a 
more or less firm compound. 

The sulphone formation from bromosulphone-chloride and benzene 
under co-operation of A/C7, is an illustrative instance hereof: 

The A/C/, is combined with the sulphone-chloride and is, therefore, 
in regard to the chloride, already far removed from the catalytic 
stage, at 25° it is however not completely paralysed, as according 
to the course of the reaction it is still capable of activating the 
second molecule (benzene). 

The sulphone formed now also unites with A/C/, and now it 
appears also from the course of the reaction that it keeps on activ- 
ating the benzene, but is, however, no longer capable of influencing 
the sulfone-chloride, for an excess of the latter exerts no influence 
on the reaction velocity. (Otivirr and Borseken, Proc. 1913 1. ¢.). 

From this case it is shown how complicated this reaction may 
become when in the reaction mixture different substances are present 
which paralyse the catalyst more or less, and that only a clear 
conception of the catalysis enables us to interpret the observations 
satisfactorily. 

Represented symbolically, we thus have here (when we assume 
that the HC/(D) does not interfere, which has also been proved by 
OLIVIER) : 


Rese Bees Cee 1) 
ae ae 
So 


The A/C/, united to C (the sulphone) can no longer reach A (the 
sulphonechloride), only the A/CZ, united to A itself can still activate 
the S-C7 bond, but much less so than free A/C/,; only the benzene 
(B) is still attainable for the A/C/,. 

I want to observe here that the paralysis starts here, presumably, 
from the SO,-group, because this occurs in the sulphonechloride as 
well as in the sulphone. 

These are just the cases, wherein the catalyst is united with one of the 
starting products, but is not entirely paralysed thereby, which have 
originated the theory of the intermediate products. 


By removing wilfully from the most favourable catalytic stage 


554 


(for instance by lowering the temperature) similar coumpounds have 
often been met with and if was imagined that the explanation of 
the catalytic phenomena had thus been found. 

Now, however, it is evident that the explanation is not given by 
the formation of these compounds, but should be found before the 
formation and that the best catalysts will be those whose dissociation 
equilibrium extends over as large as possible a region of tempera- 
ture and pressure, without any compounds being formed. 

3. In this manner, ascending by the inductive method from the 
special case of the reaction of Friepen and Crarrs (BorseKEN) and 
descending by the deductive method from the general principle of 
reciprocity (H. J. Prins), we have come to the conclusion that 
the catalytic action is situated in the pre-stage of the chemical 
wnton, 

It is evident that with this result no explanation has been found 
in the sense that now everything is completely elucidated. 

Yet, in my opinion, owing to the sharper definition of the con- 
ceptions the whole field is easier to survey (Prins le.) and the 
special cases are more readily understood, also a fundament has 
been given on which we can pursue our researches with a greater 
certainly. 

These in view of the further elucidation will have to move in 
two directions. 

Ist. It must be ascertained, as has been already done in some 
cases (L¢.), in how far the change in velocity is connected with the 
shifting of the catalyst and activated bonds in the dissociation region. 

With this may be coupled systematic researches as to the most 
suitable catalysts for specified reactions, (for instance on metals which 
are in a rapidly setting in  dissociation-equilibrium simultaneously 
with N, and H, at a low temperature in view of the ammonia 
synthesis; or on carbonates which in view of the ketone synthesis 
from acids according to Sapatier and SeENDERENS must, at about 
300°, be with those acids in the same favourable conditions). 

2ed, Those catalytic actions must be investigated where very sraall 
evergy shiftings are concerned; to this appertain in the first place 
the photocatalytic phenomena. 

The first series of researches are of a more direct practical result; 
the second series, on the other hand, are of a more penetrating 
nature, the object being to attack the catalytic phenomena in their 
last recess. 


Delft, June 1914. 


ayaa) 


Chemistry. — ‘Researches on the Temperature-coefficients of the 
Sree Surface-energy of Liquids between — 80° and 1650° C.: 
VIL. The specific surface-energy of the molten Halogenides of 
the Alcali-metals.” By Prof. Dr. F. M. Janerr. (Communicated 
by Prof. HaGa). 


§ 1. Notwithstanding the original intention to publish the results 
of the measurements concerning the temperature-coefticients of the 
free surface-energy of molten salts at the same time as the deter- 
minations of the specific gravities of the investigated salts at different 
temperatures, and in this way to give completely all data, necessary 
for the calculation of the temperature-coefficients of their molecular 
surface-energy, — it seemed desirable on account of the present 
precarious conditions, to resolve already now on the publication of 
the results hitherto obtained, and relating to the change of the specific 
surface-energies of {hose salts with the temperature of observation. 
The present uncertainty about the moment, when the now stopped 
experiments, necessary for the determination of the specific weights, 
again may be resumed in future, makes it perhaps desirable to 
publish already now the available data of the free surface-energy of 
some forty salts, and to draw the attention on this occasion to some 
general conclusions, relating to these measurements. 


§ 2. In this connection it is perhaps of interest to mention here 
also some details concerning our original tentatives, to reach the 
proposed aim by means of the method of capillar ascension-measure- 
ments, — notwithstanding the fact, that these experiments finally 
had to be given up because of reasons already formerly explained '); 
these details doubtlessly can be of use for later investigations to 
be made in this direction. 

Originally the investigated salt was introduced into wide tubes of 
heavily fusible /ena-glass, provided with rounded bottoms ; the tubes 
were heated in a bath of a molten mixture of potassium-, and sodium- 
nitrate, either by means of gas, or better by electrical current. The salt- 
mixture was filled into an iron cylinder, outwardly lined with thick 
asbestos ; its wall was provided with two diametrically opposed, 
narrow windows, which were closed by glassplates, fastened by 
means of asbestos-covered iron-frames. Through these planeparallel 


1) F. M. JAr@rr, These Proc. Comm. I. (1914). 


556 


windows the desired observations were executed by means of a 
telescope; the beight of ascension in the capillary tubes was read 
upon a perpendicularly divided seale. The liquid salt in the surround- 
ing bath was continually stirred; an arrangement was made to 
prevent as much as possible the annoying currents of hot air cireu- 
lating before the windows. 

In all these experiments it was stated very soon, that the investi- 
gated salts, when melted in the glass-tubes and on cooling again 
solidifying therein, made the tubes in most cases crack ; or at least 
they appeared on renewed heating to get soon unsuitable and badly 
damaged, thus a substitution of the tubes by new ones being necessary 
after each experiment. 

After many attempts, the tubes were arranged finally in the fol- 
lowing way, to prevent this effect. AB (fig. 1) is a tube of Jena heavily 
fusible glass, which has a conieal nar- 
rowing at a, and a sideway tube e 
with stopeock d; the wider tube ean 
be closed at its upper end by means 
of a stopper h, provided with the 
stopcock C. Just above the round 
bottom of the tube 5, a small plati- 
num crucible 7’ of about 1 cem. 
volume, hangs between three strong 
horizontal platinum-wires ; they are 
either melted into the glasswall of 
the tube, or they can be fixed to a 
platinum-ring, supported by three 
elevations in the wall of the tube. 
If in the last mentioned ease the 


tube 6 at the same time is arranged 
in such a way, that e.g. just below 
e the two parts of it can be put 
together by means of a ground col- 
lar, it will thus be possible eventu- 
ally to take the platinum-ring easily 
from the tube, and to restore it again 
after thoroughly cleaning the different 


parts of the apparatus. In every case 
the platinum-crucible 7’ needs to be 
fixed into the tube as centrally as 
possible. The narrowing at a is ground 


557 


conically ; the piece 4 (also conically shaped, ground and enlarged) 
of the heavily fusible, capillary glass-tube, can just be fixed into it; 
the capillary tube thus has the form represented in fig. 1, and it is 
cut to such a length, that it can be easily caught with a pincette 
from above through the hole 4, while at its other end it reaches 
just to a little above the bottom of 7, if 6 is caught by the collar 
a. The enlarged part of is provided at its outward side with two 
very fine, vertical canals, which thus have the function of capillary 
connections between the spaces A and JA. 

By means of a funnel with a broad and long stem, the erucible 

T is now filled with a sufficient quantity of the finely pulverised 
and dry salt; then AZ is put into the bath, and as soon as the 
salt in 7’ is molten, the carefully cleaned capillary tube is lowered 
very slowly into the apparatus, until 6 is lying just in the collar a; 
immediately the liquid begins to rise then into the capillary tube. 
Then both stopeocks C and d are closed, after the tube being put 
in such a_ position, that the capillary tube will be just vertical ; 
this may be easily controlled by means of a plummet. If now the 
air is eliminated from A through C, it will appear easily to let the 
liquid rise into the capillary tube, because the settlement of the 
pressure-differences in A and B will oceur only very slowly by the 
narrow canals in 4; in this way one can try to wet the walls of 
the tube by the liquid salt, and to eliminate the air-bubbles even- 
tually inelosed. A superfluous rising into the capillary tube can be 
stopped at any moment by means of the stopcock d. Reversely, by 
sucking at d, it will be possible, if necessary, to introduce air into 
the molten salt through the capillary tube, or to remove the liquid 
from it; also it is possible to substitute the air in AB by a neutral 
atmosphere, e.g. by nitrogen or another gas, if desired. The experi- 
ment being finished, the capillary tube 6 is removed first; the salt 
will afterwards solidify in 7 without causing the cracking of the 
olass-tube. In such a way several experiments can be made by means 
of a single apparatus. 


§ 3. Although this method of operating can be recommended in 
such cases as in principle a very suitable one, the experimental 
difficulties however appeared to be of a rather appreciable magnitude. 

One of the chief difficulties was the elimination of the very small 
air-bubbles from the liquid in the capillary tube, which appeared to 
be transported into it, whenever the liquid begins to rise into the 
narrow tube. Notwithstanding all care, this could not be completely 
prevented, and the column of liquid then appears as if broken into 


558 


a great number of pieces. It is extremely difficult, again to eliminate 
such transported air-bubbles, even in repeating the above mentioned 
way of rising and falling of the liquid in the capillary tube for a 
number of times. Almost quite impossible is the elimination of the 
air, if the wall of the tube moreover is attacked by the molten salt, 
— this wall becoming more or less rough by it: the air-bubbles 
will then persist in sticking to the narrow canal. 

Moreover the microscopical control of the glass-tubes proved 
doubtlessly that the walls of it were attacked by the molten salt 
almost always seriously te a more or less extent; this faet, in con- 
nection with the just mentioned difficulties caused by the not 
removable air-bubbles and the impossibility to determine sufficiently 
the exact situation of the surface of the liquid in 7’, were the chief . 
causes why these tentatives finally had to be stopped. In some cases, 
e.g. in that of sodiumehromate, we could obtain rather reliable data ; 
but e.g. with lithiumsalts, which will always attack the glass in a 
high degree, and just so in the case of silvernitrate, only very un- 
trustworthy numbers could be obtained. It appeared moreover to be 
very difficult, to keep the temperature constant along the full length 
of the capillary tube; this can soon be controlled by means of a 
set of very small thermometers, placed within Z at several distances 
from the bottom. 


§ 4. After this experience we thought it adviceable to abandon 
the said method completely. All numbers here given therefore are 
collected after the method formerly described by us in detail’); 
they relate to the purest salts. For the details of these experiments 
the reader is referred to Comm. I of this series. 


§ 5. Measurements of molten Alcali-halogenides. 

This series includes the following salts: The Flwordes and Chlorides 
of Lithium, Sodium, Potassium, Rubidium and Caestum, and the 
Bromides and Lodides of Sodium, Potassium, Rubidium and Cuestium. 
The preparation of the anhydrous bromide and iodide of lithium 
gave hitherto no good results, because of the hydrolysis caused by 
heating the crystallized, hydrated salts. 


1) F. M. Jaraer, loco cit. 335—348. 


Lithiumfluoride: LiF. 


Maximum Pressure 
Surface-tension 
Bere = = = z in Erg. 
: in mm. mer- ‘ , pro cm». 
cury of 0° C. in Dynes 

868.5 7.098 9463 249.5 
897.6 7.021 9360 248.0 
944 6.890 9186 242.3 
984.6 6.770 9026 238.3 
1029.4 6.634 8844 233.5 
1065 6.525 8699 229.8 
1116.5 6.323 8430 222.7 
1155.5 6.170 8226 217.4 
1208 5.976 71967 210.6 
1270 5.700 7599 201.1 


Molecular weight: 25.99. 


Radius of the Capillary tube :0.05240 


em: at 19° €: 
Depth: 0.1 mm. 


The salt melts at 840° C.; at 1150° it evaporates already rather 
rapidly, and above 1270° so fast, as to make measurements 
useless. The vapours show alkaline reaction. 


Il. 


Lithiumchloride: LiCl. 


} 
| 


Maximum Pressure 


ie 


| Surface-tension 


henperetire | hau Se hes 32 % in Erg. 

| in mm. mer- ; pro cme. 

| cury of oo c. | Dynes | 

— — al oe = = 
611 | 3.928 5237 137.8 
640 | 3.859 5145 135.4 
680 3.786 5047 132.9 
734.5 3.668 4890 128.8 
775.5 3.580 4713 125.8 
813.7 3.504 4672 123.2 
860.1 3.410 4546 119.9 
914.8 3.300 4400 116.1 
967.8 3.199 4265 112.6 
1021.9 | 3.082 4109 108.5 
1074.6 2.976 3968 104.8 


Molecular weight: 42.45. Radius of the Capillary tube: 0.05240 


The salt melts at 608° C.; at 960 


Gin: ath192 G. 
Depth: 0.1 mm. 


it begins to evaporate read- 


ily, and above 1080° so fast, that exact measurements become 
almost impossibie. The sublimed salt has a feeble alkaline reaction. 


| 


Ill. 


Sodiumfluoride: NaF. | 


Maximum Pressure 
. Surface-tension 
elas Ee 7 pl" eet eel z% in Erg. 
: in mm. mer- : pro cm?. 
cury of 0° C. in Dynes. 
fo} 
1010 5.685 71579 199.5 
1052.8 | 5.570 7426 195.5 
1097 5.445 7259 191.2 
1146.7 5.290 | 7053 185.8 
1189 5.136 6847 180.5 
1234 5.019 6691 176.4 
1263.2 4.922 | 6562 173.1 
1313 4.761 6347 167.5 
1357.3 4.628 | 6170 | 162.9 
1405.3 4.480 | 5973 157.8 
1456.4 4.330 | 5773 152.5 
1497 4.220 5626 148.7 
1546 4.070 | 5426 143.5 


Molecular weight: 42.0. Radius of the Capillary tube: 0.05223 cm. 
Depth: 0.1 mm. 
The salt melts at 990° C. At 1360° C. appreciable vaporisation 
sets in; at 1450° C. this occurs very rapidly. 


IV. 
Sodiumchloride: NaCl. 


Maximum Pressure 7 : 
Temperature << _ = ere eee es Surface-tensiony 
ee in mm. mer pro em? 
In 5 P= . | + 
euny, of, ONG: in Dynes. | 
802.6 3.580 4772.9 113.8 
810.5 | 3.572 4162.2 113.5 
820.8 | SE5O2 4735.5 112.9 
832 3.520 4692.9 111.9 
859 3.457 4608.9 | 109.9 
883.2 } 3.401 4534.3 108.2 
907.5 3.345 4459.7 106.4 
930.6 3.285 4379.7 104.5 
960.5 3.227 4302.3 | 102.7 
1999.5 Deloe 4175.6 | 99.7 
037 3.047 4062.3 97.0 
1080 2.951 3934.3 94.0 
1122.3 2.864 3818.3 91.3 
1171.8 2.761 3681.0 88.0 
| | 


Molecular weight: 58.46. Radius of the Capillary tube: 0.04736 cm. 
at 18° C. Depth: 0.1 mm. 

The pure salt melts at 801° C.; at 1080° it begins to evaporate 
already rapidly, at 1150° C. very rapidly. Between 801° and 859° C. 
the coefficient of ~ seems to be about 0.57 Erg., and to increase 
with rise of temperature. The mass shows in water afterwards a | 
strong alkaline reaction. | 


561 


V. 


Sodiumbromide: NaBr. 


| : z Sees 
| 


Maximum Pressure | 
| Surface-tension 


| 
| 
| Temperaiure = | zi Erg. 
| | in mm. mer- : * 
| | cury of 0° C. oe eMeS | 
| | “De | 
760.9 3.011 4015 105.8 
809.5 2.928 3904 102.9 
851.9 2.834 3778 99.6 
896.8 2.737 3649 96.2 
941.5 2.640 3520 92.9 
984.5 2.556 3408 90.0 
1029.4 2.449 3265 86.2 
1073.5 2.384 3178 84.0 
1116 2 302 3069 81.1 


1165.7 2.214 2952 78.0 


| Molecular weight: 102.92. Radius of the Capillar tube: 0.05240 
| cm. at 19° C. 
| Depth: 0.1 mm. 


The salt melts at 768° C.; it begins readily to evaporate at 
10002 C., and free bromine can be observed then. The sublimed 
salt possesses alkaline reaction. 


VI. 


Sodium-iodide: NaJ. 


Maximum Pressure 


Surface-tension 
ee sraneme|t fain Ere 
: : " é pro cm2, 
eirynet oie in Dynes 
| | 
705.5 2.438 | 3250 85.6 
746 2.388 | 3184 83.9 
815.5 2.291 | 3054 80.5 


860.7 2.209 | 2945 17.6 


Molecular weight: 149.92. Radius of the Capillary tube : 0.05240 
cm. at 19° C. 
Depth: 0.1 mm. 


The salt, which melts at about 660° C, evaporates soon to a 
high degree, and free iodine is observed. The sublimed salt 
reacts somewhat alkaline. 


562 


VII. 


Potassiumfluoride: KF. | 


Maximum Pressure 
y | Surface-tension 
Tene |= ee 
in mm. mer- | pro cm¢. 
cury of 0 C. in Dynes 
912.7 4.123 | 5497 138.4 
961.5 4.024 | 5365 135.2 
1015 3.898 | 5197 131.0 
1062 3.790 5053 127.4 
1097 3 701 4934 124.5 
1146.5 3.564 4752 119.9 
1185 3.450 4600 116.1 
1234 3.336 4448 PLES 
1275 3.225 4300 108.6 
1310 3.116 4154 104.9 


Molecular weight: 58.1. | Radius of the Capillary tube: 0.05002 
em. at 18° C. 
Depth: 0.1 mm. 

The salt melts at 860° C. At 1140° C. it begins to evaporate 
distinctly, at 1180° C. this goes on already rapidiy, while acid 
vapours are set free. 


VIII. 


Potassiumchloride: KCl. 


Maximum Pressure 


Temperature es eee ee eee meetin 
in ° C. in mm, mer- = : a 
cury of 0° C. | in Dynes. pro cm*, 
799.5 | 3.015 4019 95.8 
827.1 2.957 3942 94.0 
861.5 2.873 3830 91.3 
885.1 2.819 3758 89.7 
908.5 2.768 3690 88.0 
941 2.697 | 3595 85.8 
986 2.582 | 3442 | 82.2 4 
1029 | 2.484 | 3311 | 79.1 
1054 | 2.425 3233 | dee 
1087.5 | 2.361 3147 | Tei? 
1103.6 | 2.313 | 3083 IBIS 
1125 PPA 3033 72.5 
1167 2.182 2909 69.6 


Molecular weight: 74.56. Radius of the Capillary tube: 0.04736 cm. 
atgloanG, 
Depth: 0.1 mm. 


The compound solidifies after heating above its meltingpoint 


during 4 hours, at 768° C. It evaporates at 980° already appreci- | 


ably, at 1160 very rapidly. The vapours are acid, while the soli- 
dified mass shows in water alkaline reaction. The valves of the 


maximum pressure appear to decrease gradually, as a result of | 
| continuous heating of the molten mass above 1100? C. 


t 


563 


IX. 


Potassiumbromide: KBr. | 


Maximum Pressure | 
Temperature | . 7 SUP AES et sion | 
in® C. ha Gaia 
in ; - ‘ p 5 
ane 0G. in Dynes 
775° 2.702 3602 85.7 
798 2.642 3522 83.8 
826 2.585 3446 | 82.0 
859 2.504 3338 719.5 
886.5 2.450 3266 71.8 
920 2.376 3167 715.4 


Molecular weight: 119.02. Radius of the Capillary tube: 0.04728 
cm. at 15? C. 
Depth: 0.1 mm. 


The salt melts at 734° C. At 825° C. already a decomposition 
under liberation of hydrobromic acid and bromine is observed; 
| at 940° C. the salt evaporates so rapidly and decomposes to 
such a degree, that further determinations seem to be useless. 


X 


Potassium-iodide: KJ. 


Maximum Pressure H 
Surface-tension 
Homperstace = a7 Ha Erg. 
? in mm. mer- : pro cm*. 
cury of 0°? C. in Dynes 

ceils 2.372 3162 15.2 

764 2.274 3031 Teal 

812 2.183 2910 69.2 

866 2.106 2807 66.8 

873 2.097 2795 66.5 


Molecular weight: 165.96. Radius of the Capillary tube: 0.04728 
Chiat 15S; 
Depth: 0.1 mm. 


The salt melts at 681.95 C. At 750° C. already it begins to 
evaporate very appreciably, while iodine is set free. For again 
higher temperatures the determinations can hardly have any 
essential significance. 


37 
Proceedings Royal Acad; Amsterdam. Vol. XVII. 


564 


XI. 


} Rubidiumfluoride: RdbF. 


Maximum Pressure 7 
Temperature ——— 2s 


Surface-tension | 


| 
| 


| 
| 
: : z in Erg. 
° | by 
| ee | in mm. mer- | a anees | pro cm? 
| | cury of 0° (G, | ye | 
= = = : —— 1 — a ——— 
| 802.6 3.630 4839 ee 
| 847.2 3.461 4614 121.3 
| 886.8 oroel 4436 116.7 
| 936 3.220 4293 | 113.0 
985.6 3.102 4136 108.9 
1036.7 2.997 | 3996 105.2 


1085.4 | 2.910 3879 102.2 


Molecular weight: 104.45. Radius of the Capillary tube: 0.05223 
cm. at 19° C. 
Depth: 0.1 mm. 


The salt melts at 765° C. At 1000° C. it begins already to 
evaporate in an appreciable degree. 


XL. 


Rubidiumchloride : RbC/. 


Maximum Pressure H ae 
é cs urface-tension 
Teepe rate . = ee apeaniienes 
| : in mm. mer- . | pro cm?. 
cury of 0? C. in Dynes | 
o 

750 PAs BY 3642 95.7 
769.7 2.689 3585 94.2 
828.2 2.540 3386 89.0 
880 2.410 3213 84.5 
922.7 ZEB 3084 81.1 
933 2.278 3037 719.9 
961.5 2.205 2940 Tiles 
994 2.130 2840 74.7 
1036.6 2.030 2706 | es 
1088.5 1.900 2533 66.7 
1150 1.749 2332 61.4 


Molecular weight: 120.91. Radius of the Capillary tube: 0.05223 
cm. at 19° C. 
Depth: 0.1 mm. 


The salt melts at 720° C.; at 950° C. it begins to sublime 
already distinctly. Analysis gave: 29.25%, Cl and 70.75%, Rb, 
proving satisfactorily the purity of the salt. 


| 


565 


XIII. 
Rubidiumbromide: Rb£Er. 
Maximum Pressure S 
: urface-tension 
Peenealane wees cin Erg. 
in mm. mer- . pro cm’. 
cury of 0° C. zy Dynes 
| ————————————————— ———— ——— SSS = =—™ —= 
729.2 2,504 3338 87.7 
7719 2.401 3201 84.1 
831 2.301 3068 80.7 
884.3 2.200 2933 ile’ 
943.5 2.084 2718 (Breil 
985.7 2.000 2666 70.2 | 
1041 1.900 2533 66.7 
1121 1.724 | 2298 60.6 | 
| 


Molecular weight: 165.37. 


em. at 19°? C. 


Depth 


: 0.1 mm. 


Radius of the Capillary tube : 0.05223 


The salt melts at about 685° C.; at 940° C. already it begins to subli- 
me, while bromine and hydrobromic acid distinctly are observed too. 


XIV. 


Rubidium-lodide: RbJ. 


Maximum Pressure 1 


Surface-tension 


ee a Bee. 
‘ in mm. mer- é : pro cm”, 
cury of 0° C. in Dynes, | 
| 
is} | 
673.4 2.268 | 3024 79.4 
721.8 2.165 2886 15.8 
771.5 2.061 2748 PAE 
822 1.956 2607 68.5 | 
869 1.857 2476 65.1 
918 Nalos 2344 61.6 
968 1.663 | 2217 58.3 
1016 1.578 | 2104 55.4 | 


Molecular weight: 212.37. 


Radius of the Capillary tube : 0.05223 


em. at 19° C. 
Depth: 0.1 mm. 


The salt melts at 642° C. At 900° C. evaporation happens 
already distinctly; at 1000? C. it is so fast, that the measure- 
ments are influenced by it in a most troublesome way, the values 
of H seeming to be increased by the heavy vapours. 


566 


XV. 


Caesiumfluoride: CsF. 


| Maximum Pressure H é 
urface-tension 
femperaiue | ai Erg. 
; in mm. mer- : pro cm? 
| cury of 0? C. in Dynes , 
| ° i | 
| 722.5 3.116 4154 104.5 
768.7 3.011 4014 101.0 
825.6 2.872 | 3829 96.4 
877.3 2.748 3664 92.3 
929.7 | 2.624 3498 | 88.1 
985 2.510 | 3346 84.3 
1042 2.418 | 3224 81.3 
1100 2.346 3128 78.9 
| 


| Molecular weight: 151.81. Radius of the Capillary tube: 0.05002 
cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at 692° C. At 990° C. it begins to evaporate 
distmcetly. 


XVI. 


Caesiumchloride: CsCl. 


| Maximum Pressure H ; 
| Temperature Suriace tension 
| aa | ee 
| in mm, OC. | in Dynes 
|= : — | 
| 663.7 2.660 | 3546 | 89.2 
717 2.560 3413 85.9 
7711 2.440 3253 81.9 
829.6 2.315 3086 | dilotl 
881 | 2.193 2924 Sea 
934.2 2.075 2766 69.7 
979 | 1.975 2633 66.4 
1034.7 | 1.833 | 2444 61.6 
1080 1.673 2230 56.3 
| | 
Molecular weight: 168.27. Radius of the Capillary tube: 0.05002 
cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at 632? C. At 925° C. it begins to sublime; at 
1000° C. the evaporation occurs already very rapidly. 


XVII. 


Caesiumbromide: CsBr. 


| Maximum Pressure H erate ea 
urface-tension 
meuTuevalure | - | - z in Erg. 
: | in mm, mer- % | pro cm2, + 
cury of 0° C. in) Dynes | 
i S.. | 
a A ee ; | 
657.7 2.439 | 3252 81.8 
693.6 2.351 | 3134 | 718.9 
7152.5 2.231 2974 14.9 
807.5 2.132 | 2842 71.6 
858.3 2.040 | 2720 | 68.5 
915.8 1.950 | 2600 65.5 
970.6 1.865 | 2486 62.7 


Molecular weight: 212.73. Radius of the Capillary tube: 0.05002 
cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at 631° C. At 900° C. it evaporates already 
very rapidly, making the measurements very difficult. 


XVIII. 


Caesium-lodide: CsJ. 


Maximum Pressure 
Temperature e purlacetension 
bl OG, : ara ae 
mm. - : mG 
cury of 0? c, | itt Dynes 
653.6 2178 | 2904 | 73.1 
713 2.050 2733 68.8 
768 .2 1.955 | 2606 65.7 
821.4 1.860 | 2480 | 62.5 
879 1.762 | 2349 59.2 
926 1.684 | 2245 56.6 
980 1.600 2134 53.8 
1030 1.520 | 2026 tl 


Molecular weight: 259.73. Radius of the Capillary tube : 0.05002 
emi aulsouG: 
Depth: 0.1 mm. 


The salt melts at 620° C. It begins to sublime appreciably 
at 825° C. 


568 


§ 6. The temperature-cocjicients of the specific surface-energy 
of the molten alcali-halogenides. 

During these measurements, it became clear, that the shape of 
the curves, which illustrated the dependence of % and ¢, was in 
most cases much nearer to that of straight lines, than was the 
ease with most of the hitherto investigated organic liquids. However 
it must be remarked, that notwithstanding this, also in the case of 
molten salts, the y-curves could evidently belong to every one of 
the three formerly discerned possible types, while in the case of 
occurring dissociation a more rapid bending towards the temperature- 
axis could be stated, just as in the analogous cases formerly studied. 
Because of the much greater values of the maximum-pressures 
however in the here studied cases, those deviations from straight 
lines come much less to the foreground. As a consequence, in thirty 
cases of the about forty investigated salts, the dependence of y and 
¢ could be expressed with sufficient accuracy by dimear expressions ; 
for the remaining cases a quadratic expression in ¢ with three con- 
stants appeared to be adapted to this purpose to a really sufficient 
degree. 

If ¢, is the meltingpoint of the salt, then x, above this melting- 
point, can be calculated from an equation of the form: 

A%=a—b(t—t)+ct—t,)’, 
in whieh «@ corresponds to the value of y, at the meltingpoint. In 
the following table the corresponding values of ¢,, a, 6 and ¢ for 
every one of the investigated halogenides are resumed : 


Formula of ates | | 
the Salt. fs in°C. | i | b | e 

| LiF s40 | 255.2 | 0.126 | 0 

| Licl 608 140.2 | 0.076 0 
NaF 990 201.6 | 0.106 0 
NaCl 801 114.1 0.071 0 
NaBr 768 106.5 0.069 0 
NaJ 660 88.2 0.053 0 
KF 858 143.2 | 0.087 0 
Kel 780 97.4 0.072 0 
KBr 7134 88.8 0.070 0 
KJ 681 78.3 0.064 0 
RbF 765 132.0 0.131 0.00012 

R6éCl 720 98.3 | 0.086 0 

| RobBr 685 90.7 | 0.069 | -0 

| RbJ . 642 80.3 0.065 0 

| CsF 692 107.1 0.088 0.00004 
CsCl 646 91.3 0.077 0 

| CsBr 631 83.6 0.063 0 
CsJ | 620 91.6 0.056 0 


569 


Specific Surface-Energy 
in Erg pro cm?. 


760 


rere 
700" 750" 800° 850" YOU" 950° 100 190 TU 150 10 Ti Ta TW Ta Tere  —‘emperature 


Fig, 2: 


Specific Surface-Energy 
in Erg. pro cm2. 


600° 650 100" 750 800" 850" 900° 950° 0w W050 morse 7200" +“ Temperature 


Fig. 3. 


Specific Surface-Energy 
in Erg pro cm2. 


650° 700° 750° 800°850°900' 950" 000°1050 100 1150°/200° Temperature 
Fig. 4. 


Specific Surface-Energy 
in Erg pro cm2. 


650° 100° 150° 800° 850° 900° 950" wer ese”—S heMperature 
Fig. 5. 

§ 7. From these data it can be deduced in the first place, that 
in general the temperature-coefficients of the specific surface-energy 
x of these salts appear to be smadler than for most organic liquids. 
While in the last mentioned cases these values are oscillating between 


0.09 and 0.18, —as the following instances may prove once more: 
Acetic acid: 0.118. | Guajacol : (OISEL, 

Benzene: 0.136. Resorcine- Dimethylether : 0.105. 
Diethylmalonate: 0.102 Hydroquinone Dimethylether: 0.109. 
Anisol: 0.114. Pyridine : 0.125. 

Phenetol: 0.102. a-Picoline: 0.128. 

Anethol: 0.094. Chinoline : 0.104. 


— the values of 06 for these salts are situated between 0,05 and 
0,09, being thus about of the order of magnitude of the coefficient 
for e.g. ethylalcohol: 0,086. Only in the case of some fluorides some 
numbers for 6 were found, corresponding in some degree with those 
for organic liquids. (if : 0,126; RbF : 0,181; NaF : 0,106). If 
attention is drawn to the much higher temperatures of observation 
in the case of molten salts in comparison with those of the organie 
liquids, it will be hardly permitted to conelude to a principal differ- 
ence in this respect. in the behaviour of both classes of liquids; on 
the other side however just with respect to these much higher 


571 


temperatures, the enormously high absolute values of % with these 
salts, which may occasionally be more than three times that of 
water, must be considered as very remarkable. In connection with 
the data given above, we can moreover generally conclude: 

1. The temperature-coefficient 6 of the specific surface-energy 
decreases continually in the case of the four halogenides of the same 
alcali-metal, with increasing atomic weight of the halogen-atom. This 
rule holds evidently quite accurately in all the cases here considered. 

As to the absolute values of y of these salts, attention can more- 
over be drawn to the following general rules: 

2. At the same temperature t, the values x for the same halogenide 
of all alcali-metals, will decrease gradually with increasing atomic 
weight of the alcali-metal. 

3. At the same temperature ¢ the values 4, will gradually. decrease in 
the case of the four halogenides of the same alcali-metal, with increas- 
ing atomic weight of the halogen-atom. 

These relations however do not possess a simple additive character. 

Generally speaking, the Z-compounds appear to deviate more 
from those of the other aleali-metals, than these from each other; 
the A-, Rdb-, and Cs-compounds approach each other more, than 
each of these elements do the corresponding Na-compounds, while 
in the series of the first mentioned three alcalimetals, the compounds 
of K and Rb appear to have the nearest analogies to each other, 
Probably the liquid lithium-salts imay possess a higher degree of 
molecular complexity, than the salts of the other aleali-metals. 


Groningen, Augustus 1914. Laboratory for Inorganic and Physical 
Chemistry of the University. 


Chemistry. — ‘Researches on the Temperature-coefficienis of the 
free Surface-energy of Liquids at Temperatures between 
— 80° and 1650° C. VIII. The Specific Surface-energy of 
some Salts of the Alcali-metals.” By Prof. Dr. F. M. Janenr. 
(Communicated by Prof. H. Haga). 


§ 1. As a sequel to the data published in the foregoing com- 
munication, which related to the /alogenides of the aleali-metals, 
the results of the measurements made with a number of salts of 
the alcali-metals, which belong to some other series, are communicated 
in the following pages. These measurements include the following 
objects : 


572 


The Sulphates of Lithium, Sodium, Potassium, Rubidium and 
Caesium; the Nitrates of Lithium, Sodium, Potassium, Rubidium and 
Caesium; the Metaborates of Lithium, Sodium and Potassium; and 
the Molybdates, Tungstates and Metaphosphates of Sodium and 
Potassium. 

With the exception of rubidiumsulfate, which evidently contained 
some potassiumsulfate, all salts were chemically pure; the sulfates, 
molybdates and tungstates were those commonly used in this laboratory 
for the calibration of the thermoelements, and just the same was 
the ease with lithiummetaborate. For the method and practice of the 
measurements etc., we can refer to the foregoing communication. 


§ 2. 
I. 
| 
| Lithiumsulphate: Li.SO,. 
Maximum Pressure 11 
Temperature ¢ es ae ee | Suc eee 

inne G: ae 

: : pro cm?.: 

E cro Oc. | in Dynes 

| 
ie} | 

860 | 6.361 8481 223.8 
873.5 6.342 8455 223.1 
897 6.303 8403 | 221.8 
923 6.256 8341 220.2 
962.5 6.169 | 8224 | 217.4 
976.8 6.146 8194 216.4 
1001.2 6.099 8132 214.8 
1038.5 6.027 8035 | 212.3 
1057 5.987 7982 211.0 | 
1074 5.953 7936 209.8 
1089.5 | 5.923 | 7897 | 208.8 
1112 5.879 7838 | 207.3 } 
1156.5 | 5.791 7720 | 204.2 | 
1167.5 | 5.766 7687 203.4 | 
1183.5 eye TET 7649 202.4 
1192.2 | 5.718 7624 | 201.8 
1214 5.675 7566 | 200.3 


cm. at 16° 
Depth: 0.1 mm. 


The meltingpoint is 852° C.; the salt appears to be stable up 


| oe 
| Molecular weight: 109.94. Radius of ane Capillary tube 0.05240 | 
| 

to rather high temperatures. | 


573 


Il. 


Sodiumsulphate: Na,SO,. 


Maximum Pressure . 
Sui face-tension 


petupera ure laa: yin Erg. | 

: in mm. mer- é procm’. | 

cury of 0°C. ie Dyes | 

900. 6.285 8379 194.8 | 
945 6.247 8329 | 189.3 

990 6.209 8278 188.2 | 
1032 6.149 81¢8 186.5 
1077 6.088 8116 184.7 


Molecular weight: 142.07. Radius of the Capillary tube: 0.04512 
Ciipeat, 1628: 
Depth: 0.1 mm. 


The salt melted at 884° C. The molten mass, if brought into | 
water, Shows an alkaline reaction, if the temperature of the | 
molten salt has been above 1100° C. 


ll. 


Potassiumsulphate: K,SO,. 


| 
Maximum Pressure ae 
Abiea | | Surface-tension 
Hemps! Ae | in Erg 
| in mm. mer- : . 
cury of 0° C. in Dynes 
fe) 

1070.2 4.080 5439 143.7 
1103 4.048 5397 | 142.6 
1145 3.989 5318 | 140.6 
1199 | 3.878 5171 | 136.7 
1247 3.762 | 5016 132.7 
1305.5 | 3.651 4868 128.8 
1347 3.578 4770 126.2 
ile 7fil ets) | 3.529 4705 124.6 
1400 3.468 4623 122.4 
1439.5 3.393 4523 119.8 
1462.5 3.344 4458 118.1 
1490.4 3.286 | 4381 116.1 
1530.3 | 3.228 | 4304 114.1 
1586 | 3.130 | 4173 110.7 
1656 3.020 4026 106.8 


Molecular weight: 174.27. Radius of the Capillary tube: 0.05240 
cm. at 19° C. 
Depth: 0.1 mm. 


The salt melts at 1074° C., and does not dissociate appreciably 
up to 1550° C. 


Temperature 


Rubidiumsulphate: Rb,S0,. 


IV. 


Maximum Pressure 1 


Surface-tension 


in ° a x in Erg. 
in mm. mer- : pro cm*. 
cury of 0° C. in Dynes | 
° 
1086 3.760 5013 132.5 
1112 3.681 4907 | 129.7 
1144.7 3.611 4814 ies 
1195 3.520 4693 | 124.2 
1234.5 3.452 4602 | 121.8 
1289 3.368 4490 | 118.9 
1343.8 3.286 4381 116.0 
1396.8 3.223 4297 113.8 
1414.6 3.200 4267 | 113.1 
1482 3.138 4183 110.9 
1545 3.079 4105 108.9 


Molecular weight: 266.97. Radius of the Capillary tube: 0.0524 


cm. at 18° C. 
Depht: 0.1 mm. 


The salt melts at 1055° C. At about 1400° C. it begins to 
evaporate somewhat faster, and sublimes against the colder parts 
of the apparatus. It appears to contain some KjSQ4; analysis 
gave: 37,45 % SO, and 62,56 % Rb, instead of 36 %, SO, 


and 64°, Rb. 


V. 


Caesiumsulphate: Cs,SQ,. 


Temperature 


Maximum Pressure H 


Surface-tension 


insos. 

i L : ro cm? 

} Segoe oe | cangoaces, 910g 
fo} 

1036 3.170 4226 111.3 
1063 3.080 4106 108.2 
1105 2.988 3984 105.0 
1165 2.869 3825 100.8 
1221 2.764 3685 97.3 
1274.5 2.691 3588 94.7 
1331.4 2.607 3476 91.7 
1372 2.552 3402 89.8 
1423 2.482 3309 87.4 
1470 2.427 3236 85.5 
1530 2.354 3138 83.0 


Molecular weight: 361.69. Radius of the Capillary tube: 0.05223 


cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at ca. 1015° C. At 1325° C. it begins to evaporate 
in an appreciable degree; at 1440° C. very rapidly, and at nigher 
temperatures it sublimes in a rather troublesome way. 


Specific Surface-Energy 
in Erg. pro cm?. 


850° 900° 950° 100° 050° 102° 1507 200° 12501300 1950 14001950 1500 15307600 7650 770" +~Temperature 


Fig. 1. 


VI. 


Lithiumnitrate: L7NO3. 


| 
| | Maximum Pressure : 
Temperature ers So ee Sunlace tension 
Dasccetee | 0 Er 
in mm. mer- | : *. 
cury of 0° C. in Dynes | | 
358.5. | 3.334 | 4445 | 111.5 
| 403 3.260 4347 109.1 
418.2 3.240 4320 | 108.4 
445.3 3.169 4225 106.0 
492.5 3.069 4092 102.3 
| 555.3 2.956 | 3941 99.0 
| 609.4 2.872 3829 96.2 


Molecular weight; 68.95. Radius of the Capillary tube : 0.05002 
cm, at 18? C. 
Depth: 0.1 mm. 


The salt melts at 254° C. to a very thin liquid. The values 
of y are evidently szmadler than in the case of the sodium nitrate. 
At 600° C. already a decomposition, with oxygen and nitrous 
vapours setting free, can be stated. 


VIL. 
Sodiumnitrate: NaNO3. 
= = As “a 
Maximum Pressure H ; 
Temperature pe ss —— a See 
ingonG: 
is j in mm. mer- | <p yes pro cm? 
| cury of 0° C. 
———————— os 7 SS 7 —— ——— = 

32195 | 3.580 4713 119.7 
355 3.534 4711 118.1 
396.5 3.466 4621 115.9 
426.5 3.412 4549 114.2 
465.7 | 3.341 4454 111.8 
51a 3.253 4337 108.9 
559 | 3.162 4216 105.9 
601.6 | 3.086 4114 103.4 
656.3 | 2.966 3954 99.4 
693 | 2.889 3852 96.8 
738.2 2.793 3723 93.7 


Molecular weight: 85.01. Radius a the Capillary tube: 0 05002 cm. 
at 18° C. 
Depth: 0.1 mm. 


The salt melts at 312° C. At 700° C. already it distinctly 
gives off nitrous vapours and oxygen; the solidified mass gives 
in water a strong alkaline reaction. 


Potassiumnitrate: KNO3. 


Maximum Pressure 
; | Surface-tension 
ceupe yale > eG EJs ea ee 
: in mm. mer- . | pro cm’, 
Guryioh Onn) as Dynes | 

— ~~ — | — — 
380. | 3.300 4400 110.4 
436 3.168 | 4223 106.0 
480.1 3.073 4097 102.8 
534.3 | 2.942 3923 98.5 
578 | 2.841 3788 95.2 
628 | PS 7E%) 3646 91.6 
675.4 | 2.623 | 3497 87.9 
(PANG 2.506 3341 | 84.0 
771.6 2.391 3188 80.2 


Molecular weight: 101.11. Radius of the Capillary tube 0.05002 
cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at 339° C. At 760° C. already a decomposition, ana- 
logous to that observed in the case of the sodiumsalt, can be stated. 


IX, 
| Rubidiumnitrate: RbNO3. 
| ane ee a PAs 
Maximum Pressure H : 
Temperature | __ ao ee ah Le aia 
TEE : ; 
es in mm. mer- | Carre pro cm?. 
cury of 0? C. | Meals 
| 326.5 | 3.215 | 4286 107.5 
376 3.110 | 4146 104.0 
428 2.982 3976 | 99.8 
480 | 2.871 3828 96.1 
oes 2.763 3684 | 92 8 
578 2.653 | 3537 | 88. 
| 625 | 2.556 | 3408 | 85.6 
| 676.2 2.429 | 3238 | 81.4 
| 726.2 2.316 | 3088 | riley 
| | 


Molecular weight: 147.46. Radius of the Capillary tube: 0.05002 
cm. at 18° C. 
Depth: 0.1 mm. 


The salt melts at 304° C. At 650° C. it begins to decompose, 
setting free oxygen and nitrous vapours. 


X. 


Caesiumnitrate: CsNO3. 


| | Maximum Pressure H 


Temperature ¥ Surface-tension 
id gs z in Erg. 
| NOUS | se rae ite 3 pro cm?. 
| | cury of 0° C. in Dynes 
| 
| ° | 
| 425.5 2.743 3657 91.8 
459.7 2.636 | 3514 | 88.2 
5il 2.500 3333 83.7 
576.5 2.366 3154 | 79.2 
602 2.277 | 3036 76.3 
686.4 | 2.162 2882 1a 


Molecular weight: 194.82. Radius of the Capillary tube: 0.05002 
cm. at 18’ C. 
Depth: 0.1 mm. 


The salt melts at 414° C.; just as in the case of the solubi- 
lities, also in the situation of the meltingpoints of K-. Rb-, and 
Cs-nitrates an evident irregularity can be stated. At 600° C. 
already the molten salt begins to decompose. 


or 
cot hy 
(eo oF) 


Specific Surface-Energy 
in Erg pro cm?. = 


Temperature 


Fig. 2. 


XI. 


Lithium-Metaborate: LiBO,. 


Maximum Pressure H 
Temperature |—— s Surtace-lensiea 
ree (Cx ae a ae 
in mm. mer- . : 
cury of 0° C. in Dyes 
fo} 

879.2 7.442 9922 261.8 
922 7.379 9838 259.7 
967.5 7.279 9704 256.2 
1011.5 7.190 9586 253.1 
1054.5 7.108 9476 250.3 
1097.3 7.034 9378 247.7 
1149.7 6.912 9215 243.6 
1198 6.800 9066 239.7 
1249 6.638 | 8850 234.2 
1309.3 6.399 | 8531 225.8 
1355 6.252 8335 220.7 
1408 6.022 | 8029 Zen 
1457 5.750 | 7666 203.1 
1520 5.445 7260 192.4 


Molecular weight: 49.99. Radius of the Capillary tube: 0.05240 
cm. at 19° C. 
Depth: 0.1 mm. 


The salt melts at 845° C. At 1200° C. it begins to evaporate 
appreciably; the vapours show alkaline reaction (LZ0). At 1300° C. 
the volatilisation of the £/,0 occurs already rather rapidly; the y-¢- 
curve descends by this dissociation far more rapidly, than in 
the beginning. 


Sodiummetaborate: NaBOs. 


| 
| Maximum Pressure 1 | 
| Surface-tension 
Be | an Erg. 
in mm. mer- | ; pro cm. 
| cury of 0° C. | in) Dynes 
1015.6 5.762 1682 193.7 
1051.9 5.599 7465 188.3 
1096.5 | 5.378 1170 180.9 | 
1140 | 5.190 6919 174.7 | 
1192.2 4.933 6577 166.1 
1234 4.700 6266 159.7 
1276.5 4.476 5967 150.8 
1323.3 4.239 5651 142.9 
1372 4.006 5341 135.1 
1441 3.740 4986 126.2 


Molecular weight: 66.0. 


Radius of the Capillary tube: 0.05002 
cm. at 18° C. 
Depth: 0.01 mm. 


The salt melts at ca. 965° C. At 1230? C.it begins toevaporate | 
distinctly; at 1350° the evaporation goes on rapidly. 


XIII. 


Potassiummetaborate: KBQ,. 


3829 | 96.6 


Maximum Pressure 7 
Surface-tension 
Temperature -| yin Erg. | 
i x Bll : pro cm?, | 
cury of 0° C. oes Dynes | 
va 3i ae i 
992 | Bere) | | 4901 | 123.5 
1036 | 3.341 | 4454 112.3 
| 1091 | 3.062 | 4083 103.0 
1142 | 2.872 | 


Molecular weight: 82.1. Radius of the Capillary tube: 0.05002 
cm. at 18°? C. 
Depth: 0.1—0.3 mm. 


The salt melts at about 946° C. The measurements were diffi- 
cult by the great volatility and high viscosity of the substance. 
The obtained values cannot be considered therefore as being 
highly accurate. 


wo 
(06) 


Proceedings Royal Acad. Amsterdam, Vol. XVII. 


Specific Surface-Energy 
in Erg pro cm?, 


SCO* 830° CO* 950° 1000" 1050" T100° 7150" L200° T250°7500 FEO°F400" 450° F300 950 16000" Temperatu re 


Fig. 3. 
XIV. 
Sodiummolybdate: Na.MoO,. 
| Maximum Pressure | , 
Temperature | es SUrTaCe ener 
fav SG 1m oto: pty 
In mm, mer- - 50 
cury of 0° C. in Dynes 
698.5 6.091 | 8122 | 214.0 
728.5 5.975 | 7967 | 210.0 
751 5.921 | 7893 208.1 
7771 5.828 7170 204.9 
818.8 Heol 7675 202.4 
858.5 5.657 71542 199.0 
903.8 5.552 7401 195.4 
948 5.436 7247 191.4 
989.5 5.330 7106 187.7 
1035 5.224 6966 184.1 
1078.5 5.141 6854 181.2 
1121.5 5.070 6760 178.8 
| MARKO 4,998 6654 176.1 
1212 4.947 6595 174.6 
Molecular weight: 206. Radius of the Capillary tube; 0.05240 cm. 
Depth: 0.1 mm. 


The salt melts at 687° C. to a colourless liquid. 


581 


XV. 


| 


Temperature 


Potassium-Molybdate: K,Mo0,. 


Maximum Pressure 


| 

| 
Surface-tension | 
x in Erg. 


in ° C | inmm. mer- |, | 3 
| Giinys of 0°57 mene Dyn | LW Ate 
fe} 
930.6 4.310 | 5746 150.5 
977 | 4.218 | 5626 147.3 
1021 4.158 5543 145.2 
1105 4.021 5360 140.7 
1143 | 3.960 5280 138.6 
1189.3 | 3.868 5156 135.5 
1273 3.714 4950 130.0 
1286 | 3.676 4900 128.8 
1356 I) Bevesss Mel ci 123.6 
1438 3.364 4483 118.0 
1452.8 3.330 4440 116.9 
1522.3 3.205 4273 112.5 
Molecular weight: 238.2. Radius of the Capillary tube: 0.05240 | 
cm, at 18° C. | 
Depth: 0.1 mm. 


The salt melts at 919° C.; at 1400°C. it begins to decompose 
very slowly. 


XVI. 


Sodiumtungstate: Na,Wo0,. 


: = | 

Remmperatiire Maximum Pressure | Surface-tension 

corr. on i = 5 | pee | 

ray, | atm mers | in Dynes | > proemé | 

= 

710 Budg2m | 7909 | 993.3.) || 
719.5 5.909 | 7878 | 202.6 
741 5.863 7817 201.0 
788 5.718 7103 198.2 
834 5.686 7580 195.2 
879 5.579 7438 191.5 
932 eS ii 7355 189.5 
985.3 5.364 7151 184.2 
1038.5 5.280 7040 181.4 
1080.5 5.186 6913 178.3 
1133 5.073 6762 174.6 
1181.4 5.010 6679 172.4 
1231.5 4.880 6506 168.0 
1281.8 4.755 6339 163.8 
1331.5 4.663 6217 160.6 
1390.5 4.494 5991 155.0 
1450 4.405 5872 152.0 
1516.5 4.265 5686 147.3 
1559 4.171 5560 144.0 
1595 4.129 5508 142.6 

Molecular weight: Radius of the Capillary tube: 0.05113 
cm. at 16° C. 
Depth: 0.1 mm. 


The colourless, perfectly anhydrous salt melts at 694° C toa 
very clear, somewhat viscous liquid, which however at higher 
temperatures soon becomes much thinner. 


38* 


582 


XVII. 


Potassiumtungstate: K,W0,. 


Maximum Pressure ina : 
Temperature Suriac ees 
in CG: ? pro! ree 
in mm. mer- ‘ . 
cury of 0° C. in Dynes 

925 4.611 6147 161.0 
969 4.410 5879 154.1 
1012.5 4.305 5739 150.2 
1051.5 4.173 5563 145.9 
1097 | 4.056 5409 141.9 
1138.8 | 3.943 5257 138.0 
1183.2 3.832 5109 134.1 
1230 3.720 4960 130.3 
1284 3.558 4744 124.6 
1322.4 | 3.449 4598 120.9 
1366.5 3.379 4505 118.4 
| 1408.5 | 3.259 4345 114.3 
| 1458.2 3.135 4180 110.0 
| 1489 3.076 4101 107.9 
| 1520.3 3.010 4013 105.6 


Molecular weight: 326.2. Radius of the Capillary tube: 0.05201 
cm. at 17° C. 
Depth: 0.1—0.2 mm. 


The meltingpoint of the salt is 921° C.; even at 1500° C. the 
compound does not sublime appreciably. 


— —————e 


Specific Surface-Energy 
in Erg. pro cm?. 


700 


650° 700" 750" 800° 850° YOO" 950" 10001050 M0 H50° 1200 1250" 100° 13501460 14301500 19501000" 


Tempe- 
rature 


Fig. 4, 


583 


XVIII. 


Sodium-Metaphosphate: NaP03. 


Maximum Pressure 
Temperature _ | Surface-tension 

in °C. | ASE 

in mm. mer- : pro cm-. 

cury, of 02a: in Dynes 
827 5.730 7639 197.5 
871.4 5.648 7538 194.8 
927 52553 7403 191.6 
1014 5.406 ALO2S | 186.7 
1098.5 5.254 7004 181.6 
1181 5.109 6811 176.6 
1264.5 4.939 6584, 170.9 
1317 4.814 6418 | 166.7 
1434 4.511 6014 | 156.2 
1516.5 4.254 5671 147.5 


Molecular weight: 102.04. Radius of the Capillary tube: 0.05140 
cme ablboaG: 
Depth: 0.1 mm. 


The salt melts at about 620° C. At 1200° C. it begins to eva- 
porate considerably, and sublimes readily at higher temperatures. 


XIX. 


Potassium-Metaphosphate: KP0O,. 


Maximum Pressure 
Surface-tension 
Tonperfute At nee cae =) EE = x in Erg. 
, in mm. mer- ; pro cm?. 
cury of 0? GC in Dynes 
fe} 
897 4.506 6007 155.5 
942 4.395 5860 151.8 
995.7 4.346 5793 149.0 
1036 4.233 5643 146.1 
1082 4.137 5515 143.0 
1120 4.060 5413 140.3 
1167 | 3.957 5275 136.8 
1205.2 3.859 5145 133.5 
1250 3.842 5122 130.2 
1288 3.650 4866 126.3 
1344.5 3.538 4717 122.5 
1372 3.422 4562 118.5 
1412.5 3.310 4413 114.7 
1496.5 3.043 4057 105.5 
1536 2.894 3858 | 100.3 


Molecular weight: 118. Radius of the Capillary tube: 0.05140 cm. 
Depth: 0.1 mm. 

The salt melts at about 820° C.; it begins to evaporate readily | 

at 1400° C,, and sublimes fast at higher temperatures, 


584 


§ 8. The Temperature-coefficients of the Specific Surface-energy 
In connection with what was said in the foregoing communication 
about the calculation of xy, at any arbitrary temperature ¢, lying 
above the meltingpoint ¢, of the salt investigated, we only need to 
resume here the corresponding values of ¢,, a, 6, and ¢, for each salt: 


l | 
Formula of | 


eal entree eee | GPa Oe c | Remarks. 
| - Tasso, 852° 224.4 | 0.067 0 
| NaoSO4 884 196.3 0.140 0.00042 
KySO, 1074 144.5 0.066 0 
| RboSO4 1055 135.0 | 0.087 0.00007 
| CsySO4 | 1015 113.1 | 0.087 0.00006 
LiNO3 254 118.4 | 0.063 0 
| NaNO; | 312 120.7 | 0.063 0 
KNO3 339 112.9 | 0.075 0 
|  RbNO; 304 109.4 | 0.075 | 0 
CsNO3 | 414 92:0 | 0.084 0 | 
LiBO, 845 264.8 0.082 0 Decomposes 
above 1320° C. 
NaBO, 965 201.6 0.159 0 
| KBO, 946 136.6 0.310 0.00053 
Na,Mo0, 687 215.1 0.121 0.00009 
Ky Mo0, 919 152.5 0.066 0 
Na, WO, 694 204.4 0.068 0 
KiWO, 921 158.2 0.083 0 
NaPoO; 620 209.5 | 0.059 0 
Only up to 1275° 
C.; then the curve 
KPO3 820 161.2 0.069 0 bends more ra- 
pidly to the tem- 
perature-axis. 


In connection with the general rules, given in § 7 of the foregoing 
communication, we can make the following remarks with respect 
to the data given above. 

Although in these cases also, the value of yx, at the same tempe- 
rature ¢ appears gradually to decrease with increasing atomic weights 
of the aleali-metals, whose corresponding salts are investigated, we 
see that in the series of the nitrates, the lithiumsalt represents an 
exception to this rule, because its y-t-curve lies under that of the 
sodiumnitrate. It is of interest, that just in this series of the aleali- 
nitrates also other deviations of the normal arrangement are found: 
so with respect to the solubilities and the meltingpoints. About the 
relative or absolute values of the temperature-coefficient 4, nothing 
of general application can be put to the fore: evidently no simple 
relations will be found here, where the structure of the salts is already 
more complicated than in the case of the halogenides of the alcali-metals. 


: Lab. for Inorg. and Physical 
Groningen, August 1914. : J J 5 a 
: ze Chemistry of the University. 


or 


Bd 
Chemistry. — “A crystaliized compound of isoprene with sulphur 
diowide’. By Mr. G. pé Brui. (Communicated by Prof. P. van 
’ ROMBURGH). 


(Communicated in the meeting of June 27, 1914). 


As is known from the patent literature’) unsaturated hydrocarbons 
with conjugated double bonds combine in different circumstances 
with sulphurous acid. Thus, crude isoprene on shaking with an 
aqueous solution of that acid yields a compound separating in the 
form of white flakes. 

When I mixed isoprene, prepared according to Harrigs’s method *) 
(from ecarvene) and which had been purified by fractionation, the 
fraction from 384° to 38° being collected separately, with an equal 
volume of liquefied sulphur dioxide and left this mixture ina sealed 
tube at the temperature of the room, I obtained after one or two 
days a considerable quantity of a crystallized product. As a rule the 
mixture soon turns brown, but sometimes it remains colourless. 

Beside the erystals is always formed a viscous, white mass which 
on drying gets hard and brittle. In some experiments no crystals 
were deposited, but on pouring the contents of these tubes into a 
small flask it instantly solidified owing to the formation of a large 
number of crystals. 

The crystalline product may be readily recrystallized from ether. 
By repeating this operation a few times a pure, white product is 
obtained melting without decomposition at 62°.5, Presence of moisture 
is not necessary for the formation of the crystals, anyhow exactly 
the same result was obtained with tubes filled with sulphur dioxide 
dried over sulphuric acid, and dry isoprene. 

The analysis gave the following results : 

0.2016 grm. of the substance (burnt in a close tube with lead 

chromate) gave: 0.3384 grm. CO, and 0.1107 grm. H,O 

0.1612 gm. of the substance gave 0.2814 grm. BaSo, 

OE iObmGs pa ah 233 3 3»  O:3156" 5 59 

Found: 45.77 °/,C.6.10°/, H. I. 23.97 °/, 8. Il. 24.35 °/, S. 

Theory for C,H,SO,: 45.46 °/, C. 6.06 °/, H. 24.29 °/, 5. 

Determination of the molecular weight by means of the lowering 
of the freezing point ih benzene: O5491 grm. of substance in 
23.806 germs. of benzene gave a lowering of 0°.835. Molecular 
weight found: 138. 


1) D. Par. B. 59862, kl. 120, Gr. 2, 18 Aug. 1910. 
2) Ann. 383, 228 (1911). 


586 


Calculated for C,H,SO, : 132. 

Hence, the crystallized compound is formed from one mol. of 
isoprene and one mol. of SO,,. 

The substance is soluble in water. The aqueous solution has a 
neutral reaction. 

If a solution of the compound in carbon tetrachloride or ether is 
shaken with a solution of bromine in the same solvent, the colour 
of the bromine is not discharged; bromine water, however, is 
eradualiy decolourised. With dilute alkaline potassium permanganate 
a reduction sets in at once. 

As to the structure of this compound I do not as yet venture 
to pronounce an opinion. In connexion with Tnieve’s theory the 
occurrence of a compound of the formula CH, — C|CH,| = CH — CH, 


| SO, | 
would not be improbable. 
Utrecht. Org. Chem. Lab. University. 
Geophysics. — “7Vhe treatment of frequencies of directed quantities’. 


By Dr. J. P. vAN DER STOK. 
(Communicated in the meeting of June 27, 1914). 


1. The frequency-curves of barometric heights, atmospheric 
temperatures and other meteorological quantities assume different and 
peculiar forms, which can be considered as climatological charac- 
teristics and, as the number of available data increases, it is desirable 
to subject these curves to such a treatment that these characteristic 
peculiarities are represented by climatological constants. 

If we choose for this purpose the development in series-form, the 
first question is, what treatment is to be chosen for each special 
case, in conformity with the distinctive features of the quantities 
under consideration and the limits between which they are com- 
prised. The purpose of this investigation is to inquire, what form 
is to be chosen for frequencies of wind-velocities independent of 
direction, and of direction without regard to velocity. Furthermore, 
to state in how far the observed series of quantities may be regarded 
as normal- or standard-values, and the problem may be stated also 
in this way: what is the best form for frequencies of directed 
quantities assuming the form of linear quantities, and further, how 
to integrate the expression 


587 


hh' : : 
eS(h.9) RdRdO 
Ed toe ere (Lt) 


J (R.A) =? [BR sin (9@—B) — a}? + h? [R cos (AQ—Bf) — 6}? 


i.e. the standard-value of directed quantities, on the one hand with 
respect to @ between the limits 2a and zero, on the other hand 
with respect to R between the limits o and zero. 

Both problems were treated in previous communications ')”), but 
it may appear from the following that now a more principal, and 
therefore more complete, solution can be obtained than seemed 
possible a few years hence. 


2. If we wish to develop a function of one variable in an 
infinite series of polynomia 


n= 
[2 (a) =A, G;, . 
n=0 
Opa =F aaat a a2 . . ans 
the quantities a@ can be determined so that — as in the Fourimr- 
series — for the assumed limits, @ and 6 


if Dh thd = 0 


for all values of m different from 7. 


The constants A, are then given by the equation : 


A, (. daz =(rio U, da. 


The values of the constants a@ are defermined by the n equations : 


af 


[o dz = 0, fe Pale = 0G +. | OE iS ey (2) 


x 


every integral being taken between the assumed limits. 


By partial integration we have: 


1) The treatment of wind-observations. Proc. Sci. Kon. Akad. v. Wet. IX, 
(684—699). 

2) On the Analysis of Frequency-curves according to a general method, Proc. 
Sci. K. Akad. Wet. X, (799-817). 


588 


x 


. 


| UR Gi —— ais 


0 


e 


x x 


| U, « dx = a P,— Ff > =u. da 


0 0 


x 


x 
{v. ui dz =x ~,—22 9, + Ys Ps = |. dx, ete. 
‘ 0 


0 


By (2) it follows from these equations that the imposed conditions 
are fulfilled when, in the development 


| Un at de = x" —p,—n 1 —p,...(—1)—1 n(n—1) 20 (—1)rn! nts (8) 


v0 


a 


y, be given such a value that this function, as also its (2—1) first 
differential-quotients, become zero for «= and «= «and that then 


= Apy si ; 
U,, =a and fee et (=) ain cae remem Cs) 
aun 
8 B 


This simple method of determining the terms of the required series 
was indicated in 1833 by Murpny as a new method of coming to 
zonal harmonies ; in THomson and Tait’s “Natural Philosophy” it is 
mentioned in article 782. 

The method, however, is by no means restricted to the calculation 
of zonal harmonics but can easily be generalized and applied to other 
circumstances than those mentioned above. 

Instead of a complete polynomium we can also consider separately 
even and uneven polynomia; polynomia multiplied by an exponential 
factor as e-” or e-* may be used, and instead of dz we can take 
vdv (plane) or a*dzv (space) as the element of integration, whereas 
for v also quantities of another kind, e.g. siz @, may be substituted. 


3. If the limits are + 1 and —4J, it is rational to put: 


Pn = C (a? — 1)" UF = (6 (z* — 1) 


C’ being an arbitrary constant. 
Putting 


589 


nl 
C= 
(2n)! 
U;, becomes 
ee ee eae eee oth. (S) 
2(2n—1) 2 4.(2n—1)(2n—3) 


the well known form (but for a constant factor) of the zonal har- 
monie funetion and, a to (4): 


41 

eae nin! Qr+1(n!)! 

OR nS - -- 1)" dx ———— 

(2n)L J — n+ 12 ny! 
—l 
; 1 . in ; ‘ : 
utine; = Bees find, if by P, the commonly used form of 
an! 


zonal harmonies is denoted, 


D»\! 
= _(2n)- U, 
LY tere nt 
22 nInt 
from which 
4 
vad 9, 
TER Oh = = 
5 2n+-1 
—1l 
If the limits are + © and — o it is rational to choose for , 
dn 
Oy == (C7 lth, == (GF =. OH 
Pn n dian 
Putting 
C (1) 
aa an 


U,, assumes the form : 


| n(n — 1) 2 n(n—1) Yun —2 Yn a) 
G=ee|| gt — = qn—2 4 ant - 4 


ral - 
CSG. (Oe = ami 219) 
ye ) 
eisai siete =— SH nm uneven 
( a! (6) 
In—1 | 
9 
, 
Sie a ave 
genoo’ ( ) (m even) 
On ! = 
2, 


or 


and, by (4): 


+ x +a 
~ 1? ! 
U2d nt 2 n: Vy 
0h) = er dx = — uw. 
n On an 
-— o 0 


The series (6), proposed by Bruns ') and CHARitpR *), is in mathe: 
maties known as Hermirn’s function and might, if applied to 
analysis of frequencies, be called the gv, function, as proposed by Bruns. 

It is the most appropriate form for quantities as atmospheric and 
watertemperatures, barometric heights ete., moving between un- 
certain limits, and also for wind-observations if generalized for 
application to functions of two variaoles. 

In either of the cases considered above the terms of even and 
uneven power are separated automatically because 


ae, +o 
| v+1 dx = 0 and fo e—? dv =0. 
hese 1 = 


If, however, the limits are 1 and O or w and O, then such a 
separation does not take place and we must either maintain the 
complete polynomium or consider both eases separately. 


4. Considering the even polynomia separately for the limits 1 
and 0, every polynomium U2, contains only » constants and the 
development (5) takes the form: 


x 


| U2, 02” da = a2" —~, — An a2 ~, + 2? n(n—1) a4 —|, — (7) 
0 
(— 1)! 22-1 hn (n—1) ... 2 @? Gn (— 1)" 2”. nl Gna 
where 
x eb rt 
= { Wey (ihe “GPS =) P, td@... Prt = | Pn vda 
0 0 0 
az ze 
| Us, da =(— 1) 2”. ut Pn wdea . 
0 0 
Putting 
lez, 
A=-— — 
Xv da 


) Wahrscheinlichkeitsrechnting tind Kollektivmasslehre. 1906. 
2) Researches ints the theory of Probability. (Comm. from the Astron. Obsery, 
Lund.). 1906, 


we find 
Wa Nar WA or eM seun renee ag 4c. | ((9) 
whereas for g,, as the simplest expression, we must take: 
Pn = Ca?! (2? — 1)”. 
Assigning to C the value: 
1 
(4n—1)(4n—3)... 2n +1) 
the zonal harmonic function, as given in (5), is again found also for 
the limits 1 and 0. 
In the case of uneven polynomia 
Uentt = C Ar amH(e? —1ye.. 2. . 2, (9) 


which for 
1 


(4n-+1) (4n—1). . ,(2n+8) 


again leads to the expression (5). 


ai 


s 1 
Giving C' the value Bape obtain from (8) as well as from (9 
- a"! 


the zonal harmonic function in the form as commonly used. 
No more as for the limits 1 and 0, the development (7) for the 
limits a and O leads to new expressions; we have to put 


Pr C a7 e—2 


for even as well as for uneven functions, and by the formulae 


— Aye 1 H 
i — = 5 ee : (A = 2)n gen+ti ] 
on an" az 
(—1)" } o x (10) 
Uon4+1 = Sonik ene? (A — 2) aen+1 | 


we find the same expression as in § 3 for @, of formula (6), but by 
an abridged calculation. 


5. The problem, which form of development is the fittest for 
frequencies of a quantity which assumes the form of a function of 
one variable, moving between the limits 1 and O or w and 0, but, 
as a matter of fact, must be considered as a function of two vari- 
ables, is not solved satisfactorily in § 5, at least if we are not satisfied 
by a merely formal representation. 

A graphical representation of such a function is given by the 
distribution of points in a plane about a given origin, ihe element 
of integration is then, not dz, but 27RdR and the question must 
be put as follows; to find a polynomium such that 


592 
| U, Um RAR = 0 
for all values of m different from 2. 
The development by partial integration then becomes: 


| Us R2+1 dx = R2 —~,—2n R2n—2 —E, + 2?n(n—-1) R24 y, 
-(11) 


v 


(Ds Ein (nD) erect yeep 
where 


gy, =] Uakdk, 9p, = 19,kdR etc. 


if U%»,R dR = (—1) n! fotar. 


If the limits are 1 and 0, then we have to put: 
Gn = CR (R?—1)r 


and 


so that 
U2, = CAn R2n (R?—1)". 


1 
Putting C= — we tind for the polynomium : 
AL ” 


a (2n)! 


2n—1)!/ 
Oo», — R2n nC, ( : ) 
nt (n—1)! 


2n—2)) 


* (n—2)! 


R2n—-2 + ny 


Vititmes go Cie, —— (112) 


where "C, denotes the p'" binomium-coefficient of the x" power, 
further : 
1 1 1 


. . . l 
| U5, RAR = 2” (2)’f RdR=(2n)/ | R241 (F?—1)"dR= = 


0 1) 0 


nin! 


2n+1- 


This new function may be considered as a zonal harmonic general- 
ized for the case of directed quantities and might be applied e.g. 
to the distribution of hits on a target. 

The analogy of (12) with the zonal harmonic function becomes 


2n—1)! 
conspicuous if the latter (5), by multiplication by ae be 
m—1). 
given the form: 
2n—1)! ; —2! 7, (2n—4)! 
Ge ak i wy an : : ge gn? oa Aen a) yi 4 selice 
(n—1)! 2 (n—2)! 2  (n—4)! 
The expression (12) satisfies the differential equation: 


Vay 
R + 4n(n 4-1) RU, =0. 


2n 


aus ee 
BE) ee ok 


593 


For uneven polynomia ¢, has to be given the same value as (9) 
and then again the common zonal harmonie would result. As, 
however, the quantities under consideration are essentially positive, 
uneven functions ean be left out of consideration. 

If the limits are o and O, then the same reasoning holds; it is 
then rational to put: 

Gn CR tems 
Don = CA” BR e-RU'5n = C (A— 2)" RE 

Putting 

(—1y 


On 
a 


C= 


the polynomium assumes the form: 


TR 3 Den—? n*(n—1)? je. F , 
Von = R2" — n? R2N—2 + an Ren—4 — ,..(—-1)"n! . (18a) 
and 
ce oo 
Y ! 
fo RdR = 2”. utfir hak ae : 
0 0 S 


. 


In analogy with (12) the polynomium, by putting 


liye 
Ga eal 
2"n! 
may be written also: 
Rn R2n—2 R2n—4 
es Sa ES yee oes iC had as ° 2), 
Seamer Ga ne 


This new function (13) seems to be the proper form of development 
in the case of directed quantities as wind-velocities, disregarding 
direction; it satisfies the diff. equations : 

aS oe poe 
= 
a? Usn 
i 
dk? 


R -f- An RUt>, = 0 


dk 


In applyine this development, a simplification may be obtained 
pplymsg j 

by a change of seale-value: writing 7R for R and putting 

v to) to) c 


+ (2R?- a a 4+ 4(n 41) RU» = 0 


the second term with the coefficient A, will disappear as 


U', = (R?—1). 
Here J/° denotes the moment of the second order of the given 
frequency-series, 


594 


6. In the same manner as in §5 in the case of a directed quantity 
in a plane, the development appropriate for quantities in space may 
be found, e.g. for distances of stars, disregarding direction. 

The element of integration is then 47#?dR, and the development 
(11) holds good if in the left member A?"+! is written instead of 
22” and, at the same time for ¢@, 


7 = {0 Rdk 
0 


so that 
C 
Cr — R An Pn and fr = C R2n+1 e—R’, 
Vv 
Putting 
,_ (|) 
Co Qn 
U7. becomes : 
n aon 1 n on 1 on—1 
U' ne? Up —=R™ -C, =e R220, a ) R24 
. (14 
py CRED! es) 
aly) 22m! 


and 


| U*on F2dR = (—1)r. 2”. nt firn RdR = (—1)" 2°—1 nln! 


0 0 


e 


In applying this development a simplification may be obtained by 
writing HR for A and putting: 


Z 3 
HT =o’ 
then A, = 0, because 
Uo = 3), 


7. Although we may expect @ priort that the Fourier-series is 
the most appropriate form of development for frequencies of directions 
(disregarding velocity), it seems desirable in connection with the 
foregoing to show that, following the same method, we, in fact, 
come to this result. 

If 

5G SU Ct evel las 
then we may distinguish four different types of functions, namely : 


Jes F,= U sinacos a F< Uscotae (en ie Usina 


595 
For F, the development holds good: 


~. 
[ese ada = gp, sin” a — 2n x, sin?” a 4 


(Ca) 5 2n2 — IN  2o (= V)hor nN 
where 


ie 9) _ an} » 2 
i | Uda j= | Y, sinacosada ete. 
vu 


a 


Therefore, putting 


1 d 
———————— 
sin a cos a da 
2m! 
Ga = Cosme" a cose" a and) (Ci 
(2n)! 
. . . . T 
we find for the limits = and OQ: 
27. n! 
pe sin a cos a A” Gy, = cos 2na. 
(2n)! 
In the same manner: 
c 2° nn! car ; : 
Fy — — A™1 sin"-1 @ cos?"—1 a = sin 2nea 
(2n—1)! 
2". n! 
i sin at A” sin2”—! @ ¢0s2"+1 « = cos (2n + loa 
(2n)! 
2" .n! 
th @n)! cos a A” sin?'+1 @ cos?”—1 @ = sin (2n + l)a. 
an 


8. The solution of the second problem, as formulated in § 1, can 
be simplified by putting @6—PB=~y in form. (1), ie. by counting 
the angular values not, as usual, from the North-direction, but from 
NpE; this has, of course, no influence on the sums of the velocities. 

It is, however, unfeasible to apply a similar correction for the 
components a and 6 of the resulting wind, and the problem to be 
solved comes to the development in series-form of the expression : 


hh as 
ef g—la—a)>—h'(y —b)2 Fi cos G6 = y 


FL Risin O =a. 

It appears from the first of the communications cited in § 1 that, 
in following the usual method of developing, difficulties are ex- 
perienced which practically are unsurmountable. In the second com- 
munication however, it wes shown that the development (6) may 
be extended to the case of two variables 2 and y, and that such a 
function ean be developed in a series of polynomia of the form: 

39 

Proceedings Royal Acad, Amsterdam. Vol. XVIL. 


596 


F(«,y)=e—°-1"| Aoo U,+-A1.0U1+A0.1 Vit-A2.0U2+A11 Ui VitAoe Vo+et>. ](15) 
where |’ represents the same funetion of (7) as U of (x) in form. (6). 
The coefficients A are then determined by the expression: 


Aa =ef fri ty) UnVm dedy = & Sam 


—o— © 
n\m!\ 
2m+n 


xv and y, Rsin@ and Rcos 6, then, by 


Substituting again for 
to @, all uneven polynomia vanish and, 


integration with respect 


because 
sin Qn)! 
in?" a i hie ( nyt 
cos?” a 227 n'In! 
0 
we find 
Ue Vom d@ —- an - (2n)! ! (2m)! ie . »--H? 2 (HR) pe — 
x, cet 22(n-+4m) n!m! (m+n)! ! 
0 (17) 
(HR 2(m—-n—1 ) HR)2(m-+n—2) 
= mn ATES ) os --m-fn C, Ce y = (ie, 
(m+n—1)! “(m+n—2) 


i.e. the same expression as 13°, found in a different way. 
As to the determination of the A coefficients, it is expedient to 
first the case that a and 6 are equal to zero. 


consider 
It is then easily found that 
(2n)! (2n)! 
Smo= 5,1 At ET? —— 7 fe On ae 
and similarly for the V funetion 
(2m)! (2m) ! 
on= M" H? — */,)2 = 
Suze am. m! re /s) 2m .m! 
il 
Mt = — M? = —— 
2h? 2h? 


The arbitrary constant H now can be given such a value that 
P or Q=0; putting P=O, then H=A, and in the development 
only the V funetions remain. 

If a and 6 are different from zero, then it appears that (for P=0) 

S,=Q4 10 
r|s S,=3 QV 4+ 6hd7Q + hid! 

15 Q® + 45 h2b7Q? + 15 A4b'Q + Ab! 


ie) & 


or, generally : 


597 


: (2m)! F _b2Qn—i 
Son = f2n q2n at Qu 1 m( ES Adie 
aril m! Qm ; 1 
8 
Awe hi bs (Qn—? : f2m §2m |\ - (18) 
m 
rei, = =p ee —— 
kg 8 1 .3...(2m—1) 


Although, therefore, in this case the U functions do not altogether 
vanish, still the form remains the same as in (132) and (13’) because, 
as appears from (17), the polynomium has the same value for all 
terms where n+ m has the same value so that e.g. the terms with 

A40 Ayo and Ao4 
can be taken together. 

In order to investigate in how far a given collection of wind- 
observations may be considered as a collection of two independent 
quantities depending on chance, we have, therefore, in the first place 
to ecaleulate the constants a, 4,8, hand’ from the set of observations. 

In the second place the development (184) has to be applied to 
the frequency-series of the wind-velocities, thereby taking for H 
either 2 or h’ so that the term J, remains. 

A comparison between the A constants calculated in this way 
with those determined according to (18) then gives an answer to 
the question. 


9. By writing in (15) AR sin 6 and hRcos 6 for x and y, multi 
plying by RdR and integrating with respect to RA between the 
limits 0 and zero, we obtain a development representing the fre- 
quencies of the directions independent of velocity. 

The even terms Uy, and Vo,, or the product Vo, U2, then give 
rise to a series of terms of the type /, (§ 7) all of which have the 
factor cos 2ne in common. 

The even terms Us,41 Vo,41, produced by the product of two 
uneven terms have sim @ cosa as a common factor and give rise td 
terms with sin 2na, according to the functions /’, in § 7. 

The uneven terms, analogous to /’, and /’,, assume a simpler form, 
namely : 

Uont1 = Ksmacos*"a and Von41 = K cos a sin” a 
and therefore give rise to terms with sé (2n-++1) «and cos (2n-+-1) e, 
whereas all non-periodic terms vanish, except in the first term 
with A,. 

A comparison with the Fourter-series thus produced and calculated 
on the base of the five wind-constants with the Foukrer-series as 
directly deduced from the observations of direction-frequencies, then 


again gives an answer to the question. 
39* 


598 


Physics. — “Some remarks on the values of the critical quantities 
in case of association.” By Dr. J. J. van Laar. (Communi- 


cated by Prof. H. A. Lorentz). 


(Communicated in the meeting of May 30, 1914). 


1. Though this subject was treated already very fully by me ina 
paper in the Arch. Tryier') in 1908; and use was made afterwards 
(in 1909) of the contents of this paper in my Treatises on the Solid 
State *) — I wish to make a few remarks induced by a paper by 
Prof. van per Waats in These Proceedings of April 1914 (p. 1076 et seq.) 
which may contribute to the removal of the pretty large difference 
found by him (p. 1081) for the volume value of CH, for methyl- 
aleohol (2,12) and for ethylaleohol (2,76). 

Van per Waats makes namely use of values of vz, RT, and pz, 
of which he states (on p. 1078) that they would be exact by approxi- 
mation. But it has appeared from the investigation made by me in 
1908 that the “linear” dependence of the quantities RZ), and s of 
the association factor 2: (1 + 8) cannot be assumed even by approxi- 
mation. 

Not only does this hold when (as v. p. W. assumes) the volume 
of the molecules does not undergo any change on association ; when 
in other words A/ = — */, 6, + 6, = 0 — but the deviation in question 
presents itself to a much greater degree, when Ad is not = 0, as is 
certainly the case for water *) and the alcohols. 

In the cited TryLer article I started from the equation 


——) J 2 


in which @ represents the degree of dissociation of the double mole- 
cules, so that to the original '/, double molecule are found '/, (1 — 3 
double molecules and */, . 23 = @ single molecules, together ‘/, (1 + 8) 
molecules. 


1) Arch. Teyier (2) T. XI, Troisiéme partie (1908): Théorie .générale de l’asso- 
ciation de molécules semblables et de Ja combinaison de molécules différentes. 
(p. 1—96). 

2) These Proc. of April 22, June 25, Aug. 31 1909; Nov. 24, 1910; Jan. 26 
and June 23, 1911; resp. p. 765, 26, 120, 138, 454, 656 and 84. (See especially 
the third paper, p. 127—130). 

3) Already in 1899 I think I showed that the phenomenon of maximum 
density at 4° C. can be explained in a very simple way by the assumption of a 
negative value of ab, so that a double molecule would have a larger volume 
than two single molecules. [Zeitschr. f. physik. Ch. 31 (Jubelband fiir van ‘t Horr)], 


Doe 


The quantity @ appeared to have been left unchanged by the 
association, viz. =a, — the value for the case that all the molecules 
are single — everything referring to a single *) molecular quantity 
(e.g. 18 Gr. of H,O, 46 Gr. of C,H,O, ete.). For we have evidently 
(the index 2 now refers, in distinction with my Trytur article to 
the double molecules, the index 1 to the single molecules) : 


1—p\? Je! AD 2B 7 
a=|(— >-]% +2 - aa fh an ies 
= a c) - 


a, and a, = 4a,, so that we get: 


=] 
z 
= 
5 
R 
e 

| 
b 


a=(1 — @fa, +21 B) Ba, + B?a,=a 


1° 


Further : 
1—p 23 f 
ps =, BSS OS , SS a 
or ='/,6,+ 8(—‘°*/, 6, + 6,)="/, 6, + B Abd. 
The equation of state used by van pur Waats (p. 1078) is identical 
with ours, as VAN bDeR WaAAIS starts from 1 —.2 single molecules 


and 2 double molecules, together 1 mol., while we started from 
single molecules and (1— 3): 2 double molecules, together */, (1 + 6) 
molecules. Accordingly we left the quantity of substance (viz. a 
single molecular quantity, e.g. 18 gr. of water ete.) constant, and 
varied the number of mo/ecules on association from 1 to '/, (1 + 8) — 
and van ppER Waars left the number of molecules constant = 1, 
while he increased quantity of the substance from 1 to 1+ 2. 

If this is borne in mind, van per Waats’s v: (1 + 2) now passes 
into v' (now just as with us referring to a single molecular quantity 
of substance), and we get : 


RT :(l+e) a, 
P — 


(i ene Gaens? 
v—b, v 


in which therefore 1:(1-++x) is identical with our (1 + 8): 2, v’ 
with our v, VAN DER WaAAtLs putting 4/—0, and therefore identi- 
fying b with 6,. 


2. As (, the degree of dissociation of the double molecules, is a 
function of v, the dependence of the quantity @ on v will have to 
be taken into aecount in order to find the values of the critical 

1) In the cited Tryter article | made everything refer to a dowble molecular 
quantity, but I think it more practical to continue to make the different quantities 
refer to a single molecular quantity. Hence all the quantities have now been divided 
by 2, resp. 4. 


600 


3 


; f ; Op ) 
quantities in the determination of = = 0 and = = 0. The ealcula- 
v v 


tions relating to this are pretty laborious, and were carried out in 
a separate chapter (§ 5 p. 25—34) in the cited Tkyuer article (ef. 
also the above cited paper in These Proc. of Aug. 31, 1909, p. 127—130). 
We refer to this article, and give here only the results of the caleula- 
tions — again making everything have reference to a single mole- 
cular quantity. 
For vz was found: 
2 


mm 
BE APES 3m? — Qn’ (2) 
in which 
m=1 + */,8(1—8) (1+9)* a 
m=1 +4 */,8(1—8) (1+-y) + */8 1—8) 1884) (1+) 
w hile 
Ab 
PU) eae Peer ss (5) 


(p. 26 and 29 loc. cit.). 
When Ab=0 and so also gy =O, as VAN DER WAALS assumes, 
even then remains: 


m=1 + */,8(1—8) =(1+8) (1 —*/,8) 


3 1/ £ 2 2 9 a(’ (3°) 
m— 1 4-9/6 (18) +) op) (hep) (an hea 
through which for vz, with 
3m*—2n = (1+ 8)? (1—’/,8), 
is found: 
(ear 
"90 2a 
VI oN Tas (2°) 


In this the factor 3 must of course be replaced by a smaller one 
(e.g. 2,1), when & is a function of v, and varies between 6, and 6,, 
when v varies from o to 2%. 


With regard to the factor of 3b; —— which according to VAN DER 
Waats (referring namely to a single molecular quantity and not to 
a 1+ times larger quantity) would remain constant = 1 (at least 
by approximation) — we see immediately that this factor can differ 
pretty considerably from unity. For @=0 (only double molecules) 
and 3=1 (only single molecules) the factor is properly = 1, but 


for B= 7/, it has the minimum value */,. And this deviation, which al- 
ready amounts to 11 °/,, is still more pronounced when Ad is not =O, 
but has e.g. a negative value. 

For RT; we have found (p. 31 loc. cit.), again referring to a 
single molecular quantity : 


601 


8 a, 2 n*(dm? —2n) 


27 by i= 8 m® 


RI, = teen c08 (5) 


which with 44 =O passes into 


8 2 1+ 8)(1—°/,6 + */,8°)? 1—*/,8 
ee ale ( +B) ( /sf an me /4P) (52) 
Nate ase (1—?/,8) 
A 8 
If 8=1 (single molecules), then RZ, duly becomes = 
1 
8 
but for 8=0O (double molecules) RZ; becomes = 2 Xap 


But it is again immediately seen that 7), certainly does not linearly 
change with 2:(1-+8), ie. with van per Waats’s 1-2, as the latter 
assumes on p. 1078 of his treatise. 

For the remaining factor is indeed again =1 for 8=O and 
B11, but it is 3456; 3125 = 1,106 for p= */,; = 1445: 1296 = 
=e tor P= */,; and 1125 ; 1024-— 1099) for 6 = 7/,. The 
deviation can therefore again amount to 9°/,, in comparison with 
11°/, for vz, but in opposite direction. This deviation too is more 
pronounced, when 4é differs from 0. 

With regard to the value of pz, at last, we find: 

I a (8m? —2n)? (4n —3m) 


— » Oe OOM Ok 0 6 
Pk 27 6; a m? (9) 
passing into 
1k @ (1—*/,3)? (1+ 8—8p* + °/,8°) ‘ 
Pk = 55755 X — Pace (GO 
27 6, (1—’/,8) 


when Ab=0. For 
4n—3m = (1+) (1+8—36"+"/,6"). 
1 
The factor of aia duly has the value 1 both for 8 =O and 
a 1 
pies but becomes == 4617 3 3125 — 1477 for §='/;; = 379: 
oto — e430 fon) p 7/2; and —— 189. 128: — 76) for p=". 
Accordingly the deviation from unity is very considerable — for 
B='/, more than 54°/,. Hence there is no longer any question of 


an approximate equality to as VAN DER Waals supposes he 


a 
a7 8” 
may assume. (p. 1078 l.c.). And this amount can still increase for 
Ab not = 0. 


1) If it is taken into account that a = !/,d, b) =1/, by, RTk becomes as it 


; a . A : 
always did = 5? in which a and b, now refer to a double molecular quantity. 
2 


8 
27 


602 


It is therefore self-evident that when the quantities s= RT}: peor 
and 7: pz are caleulated, which occur in vAN Der WaAALs’s consi- 
derations, no linear dependence on 2:(1-+ 8), resp. 1 -+ x is to be 
expected there either. 


3. Now 
Ri wee ae ni? 
= ee re 
Pevk & 14+ 8° mn? (4n—3m) 
is found for the quantity s, passing (with Ab = 0) into 
8 2 \ (WIS ai Bom B*)* (7 ) 
= — — < = a a 
3 1p (=, eb = see) 
For 8=1 (all simple molecules) s becomes = s, = °/, (or =3,77, 


§ 


when 6 varies with v), and for 8=O (all double molecules) s becomes 
= °/, <2, hence twice the value. But here too we remain very 
far from linear dependence. 

For @='*/,; we find namely for the last factor in (7a) the value 
384 :475 — 0,808; for B='/, the value 280: 360 = 0,803; and 
for 8=7?/, the value 375: 448 = 0,837. Hence a difference of about 
DO Aeon irae 


On account of the importance of the accurate knowledge of the 


value of the quantity s for associating substances, I have calculated 
the following table. 


2 S 


B ae = ee Factor | ite X factor = S 
0 2 haga | 2 
0.1 1.818 | 0.903 1.642 
0.2 1.667 | 0.847 1.412 
0.3 | 1.5388 | 0.815 1.253 
0.35} 1.481 | 0.805 1.192 
o4 | 17420 | orent | 1.145 
0.5 | 1.333 0.803 1.071 
0.6 | 1.250 0.820 1.025 
0.7 1.176 | 0.849 0.998 
Oh |) Meili | 0.890 | 0.989 (min) 
9 | 1.058 0.945 | 0.995 
als 7a leit 1 


603 


Instead of a regular linear deerease with 2: (1)+ 8), 1.e. with 
1+ 2, values are even seen to appear <4 in the neighbourhood 
of B=1 (all the molecules single), with a minzmum at about B= 0,8 
(accurately at 80,8015), and a horizontal final direction, Le. 


d (ss 
is) =° 


On increasing association (3 from 1 to 0), s will therefore first 
become somewhat smaller than s, (= 3,77 for “ordinary” substances), 
and then (from @ = 0,7) s:.s, will become greater than 1, and increase 
to 2 for =O, when the association to double molecules is perfect. 

A straight line for s:s, (as VAN DER Waats thinks) therefore 
replaced by a line that is pretty considerably curved downward 
between the values 2 and 1 with a minimum close to 1, so that 
s:s, at first decreases there instead of increasing. 

What consequences this behaviour will have with respect to the 
degree of assvcuttion B, caleulated from the value found for s for 
methylalcohol, viz. 4,52, may appear from what follows. 

As s:s, == 4,52: 3,77 =1,2, we should find about S=0,67 or 
v=0,2 for B, according to the second column of the above table, 
when we were led by a supposed linear dependence. But when we 
also take account of the “factor” by the side of 2: (1+), we find 
about B= 0,35 or c=0,5 from the last column for the value for 


8 answering to the ratio s:s, = 1,2. 

A difference, in fact, too large to be neglected. Instead of 0,8 
single molecules to 0,2 double molecules, as vAN DER WaAats would 
find with his linear dependence, we find more accurately 0,5 single 
molecules to 0,5 double ones. The relation x: (1—a) has become 
1 instead of 4. 


4. The second quantity which plays a part in the cited paper by 
vAN DER Waats, is the quantity 7%: pe, which may be put propor- 
tional to the molecule size for non-associating substances. We now 
find for it: 

Lee 8 2 (1-8) U—*/,8+ */.8°)° 


—— oak (Sa) 


ap IP BL S83) (Sais oS) 
which with 46 =O passes into 


IL ip 8 2 n* 
== by. 


= pth Lees go) BAe) 


Dk - Ri 1+. s (3m?—2n) (4n—3m) 


We shall not discuss the course of this again, but solve from this 


604 


Q 


5 
the required value of = Ok: By means of (7) and (8) we find easily : 


ay 

8 Tienes 3m?—2n 
6) = — b = : ran. eee 5. ((Y) 
R : ie *) x m?* @) 


or when Ab=0O: 


8 Ty 1—'/.8 
6b) = — 6. = : A ¥ ye ee Qa 
One & Shae ue 


When therefore the value of 8 has been found from (7) and (7a), 
it can be substituted in (9) or (9a), and 8/p 6, is known. 
According to van per Waaus, (0) would be = 6,52 : 1,2 = 5,43 


for methylaleohol, whereas (for A= 0) the more accurate value 
with 8= 0,35 (see above) would amount to 5,43 1,084 = 5,89. 

This value is still larger than that found by van per Waats, and 
would yield 7,55 5,89 = 1,66 for CH,, instead of 2,12. And when 
4)=0 is assumed, the accurate value of (4) will be larger than 
ihe approximate one for every value of 8, because 1 — */, is always 
SS (eee ae 

It is, however, easy to see that when not (7a) and (9a) are used 
for the calculation resp. of 6 and (6), a value <1, e.g. 0,88 can 
very well be found for the factor (8m*— 2n):m? in (9), through 
which 5,48 would diminish to 4,78, so that 7,55 — 4,78 = 2,77 
would be found for CH,, in good harmony with the value found 
for ethylaleohol. 

Now (8m? — 2n):m? becomes < 1, when 


‘ 


> 
ye Or) m2 <ain. 
n 


7 
I.e. with a view to (3) 
SA US iGES ie <Us ay etal ells GF) == 
> fh (ie) (loa) (aaa 
must be, i. e. 
BULB) CL Pee) On Bie pa —<e 
< */, 8A— pi + @) =, 7, BE 8) C332) ies 
or 
(Se @) 7/5 PO SB) a 
or also 
6 — 8 =) 4 GS 8) 2) — 2) ere 
If 8 were =O, then gy would have to be < 3—/ 10, i.e. 
< — 0,162. If 8 were ='/,, then ~ ought to be < about — 0,25. 
And if @ were =1, then g would have to be << —3+ V7, i.e. 


605 


< — 0,354. As now according to (4) y= (1-+ p) Ad: (v— 3), we 
have also: 
eae ae 
b v—b 
For 7}, with v = 26, the value g:(1 + 3) follows from this for 
Ab:6. For gp resp. =0, ‘/,, and 1 we find therefore resp. the 


values < —0,16, < —0,167 and < —0,177 from this. When 
accordingly Ab:6 becomes smaller than about —‘/,, the value of 
the factor (3m? — 2n):im’ can become <1. For a value 0,88 (see 
above) it will therefore be necessary that — Ab:6 be about 0,2 — 
a value which in view of the value for H,O (which has been found 
of the same order of magnitude) is not at all impossible for methy]- 
alcohol either. 

At any rate it is seen from the above, that for associating sub- 
stances (4) cannot be put simply proportional to (7% : pz) : (s: sy), but 
that the factor (8m? — 2n):m* must be taken into account. Nor may 
for the calculation of § from s:s, simply 2:(1+ 8)=1-+ <2 be 
written for the latter ratio; another factor n° : m* (42 — 3m) must 
be added to it, which factor amounts to about 0,8 (see the above 
table) in the case AJ=O between p—O0,3 and ’=—0,5 or 0,6, which 
differs too much from 1 to be neglected. 

The error made by van DER Waats is according to § 2 owing to 
this, that he believed he could assume values for R7,: (1 +2) and 
pr, Which do not differ (at least differ little) from the corresponding 
values for non-associating substances. 

The calculation (given by me already in the cited TryiEr-article 
in 1908) teaches something entirely different: for p, (with Ab = 0) 
e.g. the deviation can amount to more than 54°/,. 

The finding of a too large value for (7%: pg): (s:s,), viz. 5,43 
instead of about 4,8 points out, that necessarily for CH,OH the 
quantity 46:6 will have a pretty Jarge negative value, namely 
about — 0,2, If 8 were about */,, then 6 would be = (1—8) */, 6, + 
+ 8b,='*/,b, + °/,6,, and from 

Ab = 3/50, by 

b ah) “he b, + ape b, ES, 
would follow 16:13 = 1,23 for-the ratio '/, b,:6,, i.e. the double 
molecules would be about 1,23 times as large as two single mole- 
cules — which is by no means impossible. 


— 0,2 


5. On this oceasion I will draw attention at the same time that 
in § 7, p. 40—42 of the cited Tryrer-article also the quantity 


606 


T dp rips 
fell *) for associating substances has been calculated by me. 
: Pp ¢ k 
When the heat of dissociation g of the double molecules may be 
put — 0, we find for 7 (see formula (28) loc. cit.) : 

n 
4n—3m’ 


=e 


or when Ab=0O: 

(LB) Seater aie) 
1+ 8— 38 + 7, 8 
in which the factor of /, both for @—O and for B=1 again 
assumes the value 1. For 8 = 1/, the value is, however, 16:19 = 0,84, 
which would make the normal value 7 descend to about 5,9. As_ 
J for methylacohol is found > 7, namely = about 8,6 (ef. Kurnen, 
Die Zustandsgleichung, p. 142, where the value 3,75 >< 2,30 is given), 
the factor of /, would have to be about J,2 instead of 0,84; i.e. 
Ab not =0, and again negative or also the value of g (see the 
full formula in Tryner, p. 42) would moreover have to be different 


ik — Te x ’ 


from 0, and that positive. 
Fontunivent sur Clarens, May 1, 1914. 


Physics. — “On apparent thermodynamic discontinuities, im connection 
with the value of the quantity b for infinitely large volume.” By 
Dr. J. J. van Laar. (Communicated by Prof. H. A. Lorgntz). 


(Communicated in the meeting of June 27, 1914). 


1. One of the principal results of the foregoing series of commu- 
nications ') has been this (cf. particularly II p. 926 and IV p. 464), 
that the quantity b,, i.e. the value of for infinitely large volume 
(hence in the ideal gas state) cannot possibly be = 4m as the classical 
kinetic theory gives for it. With decreasing temperature }, approaches 
namely more and more to &,. If in the ideal gas state 6, were 
—4m, 6b, would have to be =4m also at very low temperature 
(this kinetic result holds namely independent of the temperature), 
while in the condensed liquid state with cubic arrangement e.g. of 
the molecules, supposed to be spherical, 6, would be about = 2m’, 
in which m’ is either equal to or smaller than m, so that then b, 
cannot possibly become = /,. 


1) These Proc. of March 26, April 23, May 29 and Sept. 26, 1914 (to be cited 
as I—IY). 


607 


And yet, everything seems to point to this that actually a// sub- 
stances at sufficiently low temperature approach to the type of the 
mon-atomice substances with exceedingly low critical temperature, at 
which the quantity 6 remains almost unchanged on diminution of 
the volume from o to v,. Instructive are in this respect the tables 
in I, p. 819 and III p. 1052, and also Porncaré’s and Kameruncu 
Onnes’s remarks in the discussion of Nernst’s Report (Conseil Sotvay 
German edition, p. 241 at the bottom to 242), where it was pointed 
out that at very low temperature also the molecular heats of air 
and hydrogen would probably approach to those of monatomic gases. 

The above contradiction is now immediately removed by the 


assumption that in the rarefied gas state 6 is not = 4m, but 
simply =m (the real volume of the molecules, at most enlarged 


by a certain sphere of influence), while also in the condensed liquid 
state 5, is =m’, (m’<m) — in such a way that the idea of 
immediate contact at vv, of the quasi-spherical molecules with 
small, remaining intermolecular spaces without energy must be 
replaced by the more rational view of a compact mass of molecules 
without real interstices, unless they are considered to be the spheres 
of influence belonging to the molecules, just as for the Jarge volumes. 
This limiting state might however also be considered as a fictitious 
state, which may be approached, but which can never be reached 
entirely. But this is a question which may be left out of consider- 
ation here. 

The principal thing is that 6 always remains =m, and that on 
diminution of the volume m, therefore, only changes in consequence 
of the increased pressure under which the molecules are then, the 
less as 7 is nearer 0, till at last both at v =v, (p=) and at 
T =O the molecules will occupy their smallest volume /, =m’, 
when the atoms or atomic groups inside the molecule have approached 
each other as closely as possible. 


2. Hence we attribute, as van per Waars did in his middle 
period, when he drew up the so-called equation of state of the 
molecule, the change of 4 with v entirely to a real change in con- 
sequence of the changed internal pressure) — with rejection of 


1) For a real diminution of the molecule on diminution of v or lowering of 7’ 
speaks also the form of the empirical relation b =f (v,7) found by us — see II, 
p. 931—933, and III, p. 1051—1054. How little the later views of vAN DER 
Waats and others — in order to make the original equation of state also applicable 
to the condensed gas state and the liquid state — chi-fly by considering > as a 
function of v and 7 (of whatever nature this variability may be) — have yet come 


608 


the so-called quasi change, which would be caused by the diminution 
of the old factor 4 to about 2 in consequence of the partial over- 
lapping of the ‘‘distance spheres’. We namely assume that the volume 
available for the calculation of the pressure is immediately found by 
subtracting the volume of the molecules m from the total volume 2, 
always assuming that the kinetic energy of the moving molecules 
and molecule groups, with the permanent gradual interchange of 
the energy during the collisions, is continuously absorbed by the 
surrounding medium (see I p. 809, and IV, p. 464 at the bottom), 
and is finally after subtraction of the internal molecular pressure 
observed as ‘‘external pressure” 

It will be asked what part the so-called association or quasi-asso- | 
ciation plays in these considerations. 

Before answering this question I will first state clearly my opinion 
about the difference between association and quasi-association, which 
I hold in connection with the following considerations. We may 
briefly express this difference in the following way. 

Real association is quite individual and has a permanent character ; 
it quite depends on the chemical nature of the molecules (whether 
there are e.g. still free valencies or minor valencies present ete.). 
Water, alcohol, acetic acid are associating substances — _ ether, 
benzene, chlorobenzene ete. are non-associated substances. 

Quasi-association on the other hand in consequence of the action 
of the molecular forces, when two molecules get into each other's 
neighbourhood, and which gives rise to the formation of temporary 
“molecule aggregations’, ts entirely the same for all substances in 
corresponding states, and of transient, albeit stationary nature. 

This last form of association, which has been particularly studied 
by van per Waats, is competent to explain why with the ordinary 
kinetie view (which, when a// the active factors are taken into con- 
sideration, must also lead to the truth) not 6, = 4mis found but less. 
The theory which — evading the separate consideration of the moving 


under the notice of many, may appear again from an article by A. Wout in the 
Z. f. ph. Ch. 87, p. 1—39. This author thinks he can set everything right by an 
equation of state of the wholly unjustifiable form 


RT a c 


in which a, b, and c are constants. That it is also possible to arrive among others 
at the accurate values of the critical data by putting 6 variable with v in the 
ordinary equation of state, does not seem to have occurred to him. Also von Jiipryer’s 
many articles convey an impression of his not being at all in touch with the new 
investigations in this department. 


609 


molecules, of their collisions and their temporary aggregations — 
goes straight to its goal by imagining (see above) all the energy 
absorbed in the surrounding medium, makes it further acceptable 
that 4m would after all have to become simply m. 

But that the theory of the quasi-association can only be of any 
use in the rarefied gas state, in conjunction with the theory of the 
colliding molecules, and that the medium theory can be left aside — 
though there always remain constants undetermined (viz. the associ- 
ation constants), as we shall immediately see; and that this theory 
entirely fails for more condensed states — this is immediately to be seen. 

For if one would apply the quasi-association theory to liquids, the 
number of molecules associated to one molecule would theoretically 
continually increase, so that finally — in the limiting state — the 
whole liquid mass would have to be considered as one single asso- 
ciated giant molecule, for which the equation of state of the substance 
would then lose all its significance, as this is based on the joint 
action of an exceedingly large number of molecules, and not on a 
single molecule. What for larger volume can therefore be taken as 
the equation of state of the whole mass of the substance, would now 
have passed to the equation of state of a single giant molecule. But 
in this the separate moleeules can again be taken as unities (real 
association excluded of course) in consequence of the very slight 
mutual distances (just as for a solid substance), and the equation of 
state resulting from this will have analogous meaning as the original 
one, which holds for the gas state. Only we shall then have to take 
into account the continual change of the number of degrees of freedom. 

The theory of quasi-association, applied to condensed states, would 
therefore lead to great contradictions. While the molecules practi- 
cally behave as single ones, the said theory would lead to an infinite 
complexity in one giant molecule, with abolition of the original equation 
of state. 

While van per Waats, therefore, thought he could chiefly explain 
the deviations of the liquid state with respect to the ideal equation 
of state by the association theory, we see that exactly in this state 
this theory would lead to contradictions. It may only be applied in 
the rarefied gas state, though just there it is not necessary as an 
explanation of the deviations from the equation of state meant by 
vAN DER Waats, which would make their appearance not before 
the liquid state, but which as we saw in the foregoing articles cau 
be explained also without the assumption of quasi association. It is 
indeed necessary, however, as we shall see presently, to explain 
that then 47 can become m. 


610 


That with respect to the 4-values just liquids behave entirely 
according to the ordinary theory with 6= f(v,7) — without quasi 
association being taken into account — has appeared in my recent 
caleulations with respect to Argon. In 1V p. 458 we saw namely 
that the liquid values of 6 behave entirely according to the relation 
b= (v) derived by me (if namely 6, = 6,: vz is only raised from 
the value 0,286 obtained by extrapolation to 0,305). That the vapour 
values of 6 exhibit deviations, and even become impossible, is to be 
ascribed to the way of determination of the* vapour volumes at 
lower temperatures — since it is no longer by direet observation, 
but by application of the law of Boyin, which is not yet quite valid 
then, as I have shown in IV p. 457. 


3. Let us now proceed to examine the influence of the quasi 
association in the very rarefied gas state, by which it will be proved 
that the kinetic result 6, = 4m can no longer be maintained. 

Abbreviated derivation. If in first approximation (this is permissible 
for great v) we put the quantity 6 independent of the state of 
(quasi) association (the quantity @ is always independent of it), the 
equation of state for great v is: 

po— 6) (ee) ee eee ee (C08) 
when a fraction a of one single molecule associates to double mole- 
cules, so that there will be 1—a single and */, double molecules, 
together 1—'/, a. With very large volume the numbers of triple, 
quadruple ete. molecules can namely be neglected with respect to 
that of the double molecules. 

In this « is given by an equation of the form (see for a justi- 
fication of this and of some other assumptions the Appendix) 


Ci (1 — x)? CL 
SS Ss SS _ ‘ 
cr 1 ,v(1—’/,@) p 
as the concentration c, of the single molecules = 1—«) : (1—’/,«), 


and that of the double molecules c, = */,«:(1—*/,2). 

In this it is supposed that also the specific heat does not undergo 
any change in the quasi association, and that moreover the energy 
change may be put = 0. 

In the ideal gas state we have 7’: p= (v—6): R(A—"/,2), according 
to (1), so that we can also write: 

(l—a)? 
7 e@ 


or also, as a will always be exceedingly slight with large volume, 


C ; 
=F (v—)), 


and 7» may be written for v—b: 


If we put: 
pv - b') = RT, 
in which 6’ is the value of 6 which would be found by leaving 
the quasi association out of account — so the real value therefore 
in the usual sense —, then by comparison with (1) follows: 


v—b b b 
v— = —=v( 1 — —}(l +2/,e) =vj 1——+ 1,2], 
1-—'/,a v v ; 


sO 
v—b =v— 64+ 0.'/, 2, 
thus 
CTU Os ia) ee se og oe ee (3) 
According to (2), however, v.'/,«®= R: C, when v approaches 
to o and wv to O, so that we finally get; 
y=! R 
» = b — C he a eo te a (2) 


in whieh 64m according to the kinetic theory of the perfectly 
elastic collisions of the molecules, supposed to be spherical. And as 
C’ — the association constant — will always possess a jinite value, 
for else there would not be quasi association, we have always: 
v< b, 1. @. b'< 4m (q.e.d.). 

At the head of our paper we spoke of “apparent” thermodynamic 
discontinuities, and mean by this what follows. 

If there were no quasi association at all, i.e. if the association 


constant C’ were absolutely = 0, so that there could not exist quasi 
association at any volume, however small — then 6’ = 6 = 4mm. 


But as soon as there exists quasi association ((C’ finite), however 
slight it may be (according to (2) =O for v=o), immediately 
6 (= 4m) is diminished by the finite quantity R: C, as v X */,7= » XO 
is always finite, so that 6’ becomes < 4m. 


There is therefore discontinuity — for at an association state = 0 
for v=o, b’ can have the value 4m, and also possess all the values 
<(4m. But this is only apparent, because the diminution of 4m 
depends continuously on the value of the dissociation constant C, 
which can vary from O to any finite value. 

Now Cis not known, and this quantity, which depends on the 
entropy constants, could only be determined by statistical-mechanical 
way, when we knew ail the circumstances accurately and could 
take them into account, which determine the quasi association. In 

40 

Proceedings Royal Acad. Amsterdam, Vol. XVIL. 


612 


default of this knowledge we can therefore only say that probably 
2 


ia 
C will be such that 6’ = 4m — 7 will become about 6’=m,, in 


which m,, represents the volume of the molecules with their immediate 
sphere of influence (see § 1) — in harmony with the theory of the 
absorption of energy and transmission through the intermolecular 
medium (ef. also § 1). 

If an analogous image is wanted: the old ballistic theory of 
the rectilinear motion of the colliding molecules is in the same 
relation to the modified theory, “in which the temporary mutual 
influencing of the molecules is considered which will take place at 
every impact, or (what comes to the same thing) to the medium 
theory — as the consideration of the effect of a ray of light, 
after it has passed through a narrow aperture without taking the 
inflection into account, so that only that part of the space behind 
the aperture would be affected by the light which is in the direction 
of the ray — is in relation to the complete consideration of the light- 
effeet with observance of the diffraction, in which therefore the 
whole space behind the aperture is affected by the light, and of 
which it is possible to determine the distribution of the intensity. 


Appendia. Complete derivation’) of (A). 
If a fraction x, of 1 mol. is temporarily joined to double molecules, 
a fraction v, to triple molecules etc., we have therefore: 
n,—1—2#,—2,... single mol. ; ,=%*/,2, double mol; 
n, ='/, «, triple mol.; ete. 
If further generally : 
b=n,b, +n,b, + 7,6, +.., 
then 
= (1 —a, — 2, — 222) 0; Ey OF, Oe ee 
or 
OD me (Des ig) eg Onan) ere 
In this 6, —*/,6,= A, 6 represents the change of +, always when 
a half double molecule dissociates to a single molecule; 6, —*/, 6, = A,b 
the change of 6, when one third triple molecule dissociates to a single 
mol.; ete., so that we can also write: 
b= b, — 2x, 4,b—a2x, A,b — ete. ee to (a 
That a does not change in consequence of the association, is known. 
For three kinds of molecules e.g. holds namely : 


1) Already derived by me in 1908, but never published. 


613 


@=n,?a, + na, + n,’a, + 2n,n,a,, + 2n,n,a,, + 2n,n,a,, ; 
meawnich @, = 40. , a; = 90. 0, — 20. — 3d, and @,; = 6a;, 
so that we get: 

a=—n,?a, + 4n,?a, + 9n,?a, + 4nyn,a, + 6n,n,a, + 12n,n,a, 

= (n, 4+ 2n, + 3n,)?u, =a, , 
as n, + 2n, + 3n, = (1 —2,—a,)+2a,+2,=1 


We may therefore write: 
(» a 5) (CES bao REE. erties arr () 
v 


in which 6 is given by («), and (see above) 


C= =n =) Sy —— ol Giese a vaso to 64) 

The following equations hold for the dissociation equilibrium of 

ihe double, triple ete. molecules resp. (cf my alveady frequently 

cited Teyler paper 1908: Théorie générale de association ete., 

p. 5, and also These Proc. of June 23, 1911 (Solid State VII), for- 
mula (28)): 


(l—a,—a,—...)? C 2 tt 5—%/RT ete eee RY 


- pe Tas ee 
= ere 3 e/ a pte 

re ees MO Gea ea Ge ee 
role? Wi a (p+4/o)? 


or taking the equation of state (@) into account : 


Bee ee By 
(1 Uyg— Lye ) a C, Th oe b/ RT e— 9. 2Agb : (e—b) (y— ) 


af ic R 
beep NN 7 papers tea) 
(L—#,—#,—-. ) wee 2778 6 —WRT ¢ - 9. 3Agb : (v—b) (y —)? 
1 a 78 
is Ws, vv 


. . . . ry . . . > . . . i . ry . . . 


in which C,, C,, ete. are the dissociation constants resp. of the 
double, triple ete. molecules; y,, y,, ete. the changes of the specific 
heat in the dissociation, divided by R, viz. y, = (2k,—A,): R, 
Y, = (38h4,—A4,): R, ete.; 9,, qs, ete. the heats of dissociation (energy 
changes) 2(¢,))—(e2)o, 3(€,)> —(@,),, ete.; Ab, Ad, ete. the variations 
of 6 already introduced above, which must now resp. be multiplied 
by 2, 3, ete., the above equations referring to n-fold molecular 
quantities, and not to a single quantity. 

The first member contains the relations of the molecular concen- 
trations, viz. 

40* 


é* (n,:2n,)? 2,7 (1—#,—a,—...)? 
= = 7 Tt i 

ce Dn Oe nO ile 's (2) 

e,* _ (n,: &n,)? De (l—#,—2#,—...)* 
== ry ? 

cn Mae eaHey role Vion ald 


ete. (for Yn, has namely been put 0). 
For the dissociation constants C,, C,, ete. holds: 
log C, = — ¥. + Ay + (log R — 1), 
log C, = —y, + 4, + 2 (log R— 1), 
etc., in which A,y, 4,7, ete. represent the variations of the entropy 
constant, divided by A, viz. A,yj=(2(,),—(m;),): 4 Ap = 
= (3 (,), — (1,).): KR, ete. 

If we now put all the quantities y and g=0, which is allowed 
for quasi association (otherwise we only think the terms referriny 
io it included in the dissociation constants, e. g., CT? ¢ t/RI= 
= C,’, ete.), then for large volumes, where «,, 2, ete. will be slight: 

: S C, e— 4 2dgb :(v—b) (y—b) 
ie vy Kh 


1 y; 
_— A e—4.3A3b : (v—b)(y — B)? 


ne - 

or as also Ab: (v—bd), A,b: (~—), ete. will be very small for large 
v, and v may be written for v — b: 

. R 1 ma 

“itr m ee C, ai CLC) er mae 
of which the first equation is identical with (2) of § 3. 

We further see, what we have already immediately put in our 
abbreviated derivation, that really for very large volume .,,.7,, ete. 
may be neglected by the side of «,, and that therefore the consider- 
ation of the dowble molecules suffices with disregard of the numbers 
of triple and multiple molecules. 

If we now again compare the equation (3) with (p+-¢/,2\v—bJ=RT 
(the latter therefore without taking quasi association into account), 
then (see also (@) and (y)): 

v—b = y—b,4+2,4,b+2,A,6 +... 
6 1—*/,7, — ?/,0,—-- 


hence with neglect of z, ete. by the side of w,: 


v—b,—wx,A,b b, 4b ; 
v — = ——. ——— ore + fre . 


; 


z —. 
SR 


or 


615 


7) 


l 


b! = »—b,--2, 4,6 + v.*/ 


ob 


In this the infinitesimal quantity ,4,b (also when A4,/ is finite) 
may be neglected by the side of 6, and the also finite quantity 
Ho /s2,, and we get: 

OO Ue eae, 


identical with (3) of § 3. For v.'/,2, the value R: C. 


, follows then 


again from (), and the conclusions are further as in the cited paragraph. 


Fontanivent sur Clarens. 


Chemistry. “Ourrent Potentials of Electrolyte solutions’. By 
Dr. H. R. Kruyr. (Communicated by Prof. Ernst Coney). 


(Communicated in the meeling of June 27, 1914). 


1. For a proper understanding of the reciprocal action between 
electrolytes and colloids the knowledge of the capillary-electrie 
phenomena is indispensable’). Researches on the influence of the 
electrolyte ‘concentration in these phenomena have indeed been 
earried out of late years; Pwrrin*) and Enissarorr *) studied the 
electric endosmose of electrolyte solutions, Burron *) determined the 
influence of electrolytes in various concentrations on the cataphoresis 
whilst there already exists a vast material on the capillary-electro- 
meter and the dropping electrode’). The recent investigations were, 
therefore, chiefly concerned with the measurement of the phenomena 
of motion in consequence of a supplied electric tension ; the reverse 
phenomenon, however, namely the occurrence of an electric tension 
in consequence of a moving electrolyte solution has been but little 
studied "). The former investigations on these current potentials 
(generally, though less accurately, called “Str6mungsstréme”) are 
restricted to pure water. True, Crwonson’) states that electrolyte 
solutions cannot produce current potentials, but from the quoted 
treatises of Gourk pe ViILLEMONTEL *) it appears that the latter only 
1) For full details of this problem see H. #RmUNDLICH, Kapillarchemie, Leipzig 
1909 in very condensed form H. R. Kruyz, Aanteekeningen Prov. Utr. Gen. 3 June 
1913 p. 9 and Chem. Weekbl. 10, 524 (1915). 

2) Journal de Chimie physique 2. 601 (1904). 

5), Z. f{. physik. Chem. 79, 385 (1912). 

), Phil. Mag. [6] 11, 425; 12, 472 (1905) and 17, 583 (1909). 

5) Detailed literature statements in Cuwo.son, Lehrbuch der Physik IV 1. 

6) The most important investigations of recent times are those of CAMBRON and 
Orrrincrr, Phil. Mag. [6] 18, 586 (1909); GrumBacH, Ann. de chim. et de 
phys. [8] 24, 433 (1911) and Ruiry, ibidem [8] 30, 1 (1918). 

7) |. ce. note 5. 

8) Journ. de phys. [3] 6, 59 (1897). 


616 


investigated solutions of CuSO,, ZnSO, and NiSO, in the concentra- 
tion of 10 grams per litre. Because current potential and electro- 
endosmose are so to say each other’s reflected image *), one 
may rather expect that the electrolyte concentration will make 
itself felt in a similar manner in regard to those two phenomena. 
As Euissarorr (I. ¢.) found that even exceedingly feeble electro- 
lyte concentrations strongly diminish or suspend the  electro- 
endosmotic transport, we can only assume from the negative result 
of Gourté pe Vitiemontée that in the concentrated solutions used by 
him the potential is already lowered to about zero. Rufty’s result *) 
have also confirmed this conclusion. 

Grumpacn *), who investigated the influence of non-electrolytes on 
the current potential, has not used pure water as comparison liquid 
but a KCl-solution of the concentration 1 millimol. per litre and in 
this manner obtained positiv results. In the investigation here 
described I have made use in many respects of the experimental 
methods mentioned in GruMBACH’s paper. 


9, 


KEM 


Yi); 
CL 


A i 

—— SS SSP 5 & A 
Bee, EI el 

OW, We) 

QO oO 

f aR & 

Q oO 

=| iB; 


Fig. 1. 


*) Vel. SaxEn, Wied. Ann. 47, 16 (1892). 
=) JE Os 
) I ee 


Vv 
I 
I 


3 


617 


2. Apparatus. In tig. 1 the apparatus used is represented 
schematically. The liquid serving in the experiment runs from flask 
F into flask F, through a doubly bent glass tube Aap, which is 
partly drawn to a capillary. Into the three-necked Wouter flask /,, 
which is closed by means of rubber stoppers with copper wire 
ligature, arrives also (1) a tube @ through which air can be pressed 
and (2) an electrode #,. In the other flask /’, is found an electrode 
&, and a thermometer 7. The electrodes are Ag-AgCl electrodes. 
A silver wire is fixed into a glass capillary by means of CaiLLrret- 
wax, The protruding end is electrolytically covered with AgCl 
according to the indications given by JAHN *). 

A constant pressure above the liquid in flask /’, is obtained as 
follows: by means of a cycle foot-pump mereury can be pressed from 
the reservoir /, into R,; the pressure thereby generated is read off 
on the open mercury manometer. As owing to the transferring of the 
liquid from /, to /', the pressure would diminish a little during 
the experiment, it is kept constant by means of the arrangement 
CD by turning the handle C. 

The measurement of the potential differences between the electrodes 
E, and E, was carried out by the compensation method of Pogary- 
porFr-pu Bots Reymonp. A galvanometer could not be used as a zero 
instrument because the strength of the current passing through the 
instrument is exceedingly small in consequence of the enormous 
resistance in the battery /F,. Hence, a capillary electrometer 
(KEM in fig. 1) was used, which was fixed to the object table of 
an ordinary microscope; the axis of the microscope was, of course, 
placed horizontally. The readings were made using of an ocular- 
micrometer, objective 4c (Reicnert) and Huyeens ocular 1. 

The following serves to further explain the figure. S, is a key 
for cutting off the short circuit of the capillary electrometer; A in- 
diecates that this is connected with the earth. As working element 
are used one or more accumulators Acc whose tension was determ- 
ined by comparison with a Weston standard-cell, which was placed 
in a thermostat at 25° (WNE). By O the different current inter- 
rupters are indicated; by O, the electrodes #, and £, can be brought 
into short circuit, which was always done during the time that no 
observations were made. By Q, the current of the working cell is 
twitched in; QO, annables to introduce at will one, two or four 
accumulators as a compensation battery. QO, renders it possible to 
take up in the circuit either the standard cell or the battery 1, /’,. 


1) Zeitschrift f. physik. Chem. 38, special page 556 (1900). 


618 


In order to protect the Ag-AgCl-electrodes from the light, the 
flasks /’, and /, are externally coated with a film of red gelatin 
obtained by inserting them in a solution of gelatin to which a little 
eosine had been added and which had just started to gelatinise. 
Moreover, they were always protected from direct daylight. 

3. Method and preliminary experiments. The measurements were 
made a few minutes after the pressure had set in. A number of 
measurements at different pressures were always made. When between 
{wo measurements the liquid had to be pressed back from flask /, 
to flask 7’, (for which at @ the connection with the pressure arrange- 
ment could be broken off and an oil suction pump attached), no 
measurements were executed at suction pressure. 

From Grumpacn’s experiments we notice that the value of the 
current potentials varies a little during the first days after the con- 
struction of a battery /,F,. 1 repeated one of his observations, also 
with the object of comparing the results obtained with his and my 
own apparatus. 

Table I contains the results of a series of measurements carried 


TABLE I. 
p iE E P| ae ae 
em mercury) millivolts P cm mercury , millivolts | P 
11 March = t= 14° | 622 | 253 4.1 
61.2 271 4.4 SIe | 218 4.3 
86.4 367 4.2 average 41 
54.8 236 4.3 yj Mes March Le OS 
70.8 315 4.4 82.2 310 | 3.8 
average 4.3 85.2 323 | 3.8 
12 March 1 1 ele 22 280 3.9 
43.2 201 tel “eos | |) 1236 ll ene 
57.2 240 4.2 average 3.9 
68.1 | 280 41 16 March = t= 14° 
average 4.2 | 86.2 | 341 | 4.0 
13 March = t= 14° 70.2 | 284 | 4.0 
85.2 | 350 4.1 58.8 240 | 4.1 


73.2 | 302 | 41 | average 4.0 


619 


out with a solution of the concentration 1 m. Mol. AC/ per Liter. 
The battery was filled March 11'". P indicates the pressure, E the 
current potentials. 

From this we notice that the apparatus acted splendidly. The 
potential per em. mercury pressure has each day a constant value, 
but varies the first two days. On the third day the terminal value 
is attained. 


4. Ieasurements. In this paper a series of measurements is com- 
municated, the object of which was to ascertain the influence of 
some solutions which differed in the valency of the cation. Therefore 
solutions’ of the chlorides of A’, Ba’, and Al" were used. As 
solvent was always used so-called “conductivity water”. The very dilute 
solutions were made by diluting a standard solution. Ali measures 
used in this investigation were carefully calibrated or recalibrated. 

In order to shorten the time of these tedious measurements 
they were all executed 20 hours after filling the cell. True, the 
constant terminal value is then not yet attained, but the difference 
is comparatively small and the error introduced is the same in all 
measurements. Moreover, the inaccuracy caused thereby is without 
influence on the tendency of the conclusions presently to be drawn, 
in itself a good reason for proceeding to this measure of enormous 
time saving. Moreover, several sets of flasks were used, in such a 
manner however that, for instance, all the ACZ/ solutions were 
measured in the same set. Finally, the sets were compared mutually 
in which the solution of 100 a J/o/. (micromol ='/,,,, millimol) A C7 
p. L. served as comparison liquid. With both apparatus was found 
exactly the same value for the potential per unit of pressure. 

In the subjoined tables, the concentrations in the first column are 
given in « mols. p. L.; in the second column is found the current 
potential #7 in millivolts per unit of pressure (ecm. of mercury) under 
which the liquid was forced over. This value is always the mean 
of two ov more measurements whose differences were of the order 
of those in Table | (generally much less than those). 

When in the tables no sign is indicated at the potential value, 
the condition (as with pure water) is such that the electrode E, in 
fig. 1 is negative. In the A/C/, solutions a change of poles took 
place, hence the potentials following are indicated by ++. 

The results of the tables If to [V are represented graphically in 
fig. 2. Fig. 3 also gives the curve for A/C/, on a larger scale. 


-300 -300 


200 


—200 


= 100 —100 


a 
100 200 300 


400 500 10 
conc. Mol p.Li. conc. 4 Mol p.L, 


+100 


J 
Fig. 2. Fig. 3. 
TABLE II TABLE III 
| KCI | BaCh 
| = | | 
Cone. | | Conc. 
in yMol | Bi | in #Mol Pa 
| P P 
Dale | Puls 
| 
= = : —| a 
0 about 350 | 10 139 
50 102 | | 25 79 
100 | 51 | 50 44 
250 | 23 | | 100 25 
| 
500 | 12 | 200 9 
1000 | 4 | 1000 1 
40000 no exchange of 
poles 


621 


TABLE IV 
| AICI, | 
be | 
| Conc. | 
| in »Mol = 
| p. L | 

0 about 350 
| 0.5 52 
1 | + #2 
2 le se | 
3 + 129 | 
| 4 Le == 100 | 
| 10 Hee ease | 
| 100 Ib eectaves 
500 ah 4A | 


5. On considering these results we notice, of course, first of all the 
great influence of the valency of the cation; as this gets higher the 
capillary gets more strongly discharged at an equal concentration. This 
had also been observed by Enissarorr when measuring the electric 
endosmose and may be noticed with Risry from his experiments with 
uni- and bivalent ions. The latter has observed a change of poles only 
onee, namely with copper nitrate and that only at a high concen- 
tration’). In the case of A/C/, about 0.8 uw mol. or about O.1 mg. 
per liter appears to be sufficient to lower the current potential from 
about 350 mV. to zero. It seems remarkable that this charge reversal 
does not take place with AaC/, (see Table II) neither with ZnSO, 
or CuSO, (Rifty) nor with substances with a univalent cation. 

Still more striking is the fact that according to Exissarorr, the 
electro-endosmotic transport requires, in a glass capillary, 100 micro- 
mols of Al: to be reduced to 0 without a reversal occurring, whereas 
the same investigator, although attaining the zero point, with a quartz 
capillary, at about the same concentration as required in our research 
{he found 1.6 @ mol. $ Al, (SO,),| could not even then notice a 


reversal of the transport direction. This creates the impression that 


1) The exact concentration cannot be made out from his experiments. In any 
case, however, it lies above 900 « mol p. L. 


622 


in that research secondary influences come to the fore; perhaps the 
powerful electric field in which the measurements are executed is 
not without influence on the capillary itself. Only the quadrivalent 
Th-ion was capable of causing a charge reversal. 

The results obtained here are in harmony with the general theore- 
tical points of view. The electric double layer in the capillary, in 
the case of pure water consists of 'OH-ions at the side of the glass 
wall and ‘H-ions at the side of the liquid in consequence of the 
selective ion adsorption of the glass wall which always adsorbs the 
‘OH-ion more strongly. From the electrolyte solutions the cations are 
absorbed more eagerly than the anions so that the charge gets lowered. 
If this adsorption for KCI, BaCl, and AICI, is such that solutions of 
the same molecular concentration are absorbed about equally, it is 
conceivable that the three times more active Al-:-ion requires a much 
lesser concentration than the K'-ion in order to attain an equal 
potential reduction. 

If once the capillary is charged reversely the adsorption of the 
Cl-ion, which carries a charge now opposite to that of the capillary, 
seems to predominate. The positive charge now soon attains (at 3 j mol.) 
a maximum value, and than decreases, but only slowly, because the 
discharging ion is univalent here. 

In agreement with the theory are also the resalis of Ruiry '), for 
instance that the salt of a heavy metal has a stronger discharging 
action than that of a lighter one (Cu and Zn, at least in the small 
concentrations). A cation of a heavy metal is known to be adsorbed 
more strongly than that of a light one.*) 

Moreover, the behaviour in the case of CuSO, and of Cu(NO,), is 
in agreement with investigations as to the adsorbability of those salts *). 
The influence of the anions is also observable in Rusry’s results and 
appears to have an effect corresponding with that in the ease of 
AICI, just described. 

The question whether the organic cations also behave according to 
the theoretical expectations is being considered. Several other solutions 
of electrolytes in water as well as in mixed solvents *) will be 
investigated. 

Utrecht, June 1914. van ‘ Horr-Laboratory. 


MHL @ 

2) Morawitz, Koll. Beih. 1, 301 (1910). 

5) Freunpuicu and Scuucui, Z. f. physik. Ghem. 85, 641 (1913). 

*) Of these have also already been measured a few series in connexion with 
the researches of Kruyr and van Dury, Koll. Beih. 5, 269 (1914). 


623 


Chemistry. — “Electric charge and limit value of Colloids’. By 
Dr. H. R. Kruyr. (Communicated by Prof. Ernst Coney). 


(Communicated in the meeting of June 27, 1914). 


1. The present conception as to the relative stability of the sus- 
pensoid system and the way in which it may be suspended has been 
developed according to the following train of thoughts. 

Harpy *) and afterwards burton *) have undoubtedly established 
the fact that this relative stability falls and stands with the electric 
charge of the suspended particle. Indeed, the permanently suspended 
particle that exhibits a vivid Brown’s motion, has a cataphoretic 


oF : Volt—. re 
mobility of the order 2—4 uw per second and per eM. ;if by addition 
e.M. 


of an electrolyte one diminishes the relative stability, this velocity 
also decreases and therefore, the electric charge of the particle has 
evidently decreased also. The ‘iso-electric’” point, where that charge 
seems to have become zero, coincides with the moment of the small- 
est stability. Since the research of Wuitney and Ossr *) we know 
moreover, that with the repeal of the stability (the coagulation) is 
coupled a combination of the coagulating ion with the particles, and 
by Freunpiicu’s *) researches we arrived at the knowledge that these 
phenomena are described quantitatively by the equation of the 
adsorption-isotherm. 

From these elements is built up the theory that the particle owes 
its charge to the selective ion-absorption in its boundary layer and 
loses it by tke selective adsorption of the oppositely charged ion of 
the coagulating electrolyte. As specific properties of the adsorbent are 
usually of but very subordinate influence on the order of the charac- 
terizing quantities in the adsorption, the action of diverse electro- 
lytes on all capillary-electric phenomena ought to exhibit the same 
order, which the researches as to the electro-endosmotic phenomena 
compared with those of the coagulation of colloids have indeed 
confirmed. 

It now occurs to me that the researches on the current potentials, 
particularly those which have been communicated in the preceding 
paper, are capable of furnishing us not only with a new proof of 
that equality of order, but also demonstrate that the influence which 

1) Z. f. physik. Chem. 33, 385 (1900). 

2) Phil. Mag. [6] 11, 425; 12, 472 (1906) and 17, 582 (1909). 

8) Z. f. physik. Chem. 39, 630 (1902), 

) Zeitschr. f. physik. Chem. 73, 385 (1910) and 85, 641 (1913), 


624 


electrolytes exert on the charge of a glass capillary is quantitatively 
the same as that exerted on the colloidal particle during the coagulation. 


2. As regards the order of the ion-actions, it has been pointed 
out in the previous paper that the ions discharge more strongly, 
when their valency is higher and that the heavy metals exert more 
influence than the light ones of equal valency. It is well-known 
that the limit values for the coagulation of suspensoids just exhibit 


the same peculiarities. 


3. In order to make a quantitative comparison it should be first 
observed that the limit values for KCl and BaCl, in the same sol. 
are generally in the proportion of about 60: 1. In contact with 
either of these solutions the charge of the particle thus gets equally 
diminished. We may, therefore also expect that the charge of a glass 
capillary will be lowered by a solution of KCI to the same extent 
as by the sixty times weaker BaCl, solution. Hence, when from the 
tables 1 the preceding paper we calculate the charge in concen- 
trations of KCl and BaCl, in the said proportion, those should be 
equal if the idea as to the limit value just revealed is a correct one. 

The caleulation of the charge is possible according to the theory 
developed by Hetmno.rz'). The current potential is sequel to the 
electric double layer formed at the wall of the capillary and is 
related to the electric moment J/ as follows. 


w 
f= WP 6 S|) Sea 
y) 


in which w represents the specific resistance and 1 the constant of 
the internal friction whilst P represents the pressure employed. For 
comparison purposes we can consider the electric moment of the double 
layer just as well as the charge ¢ per unit of section, as it is in 
inverse proportion therewith. 

We write equation (1): 


If now we indicate the quantities relating to a BaCl,- solution 
with the index /, those relating to the 60 times more concentrated 
solution of KCl with the index /, then on the strength of the above 
considerations we must get 


EN Mb ef ie 
al wy \PJe wx 


(! Wied. Am. 7, 337 (1879). 


625 


As we only have in view very dilute solutions, we may put 
Hy = 7 (namely = yu,0). From this follows 


or in words: the relation of the current potentials of two electrolyte 
solutions whose concentrations are related as in the limit values of 
colloids are inversely proportional to the specific resistances of those 
solutions. 

Meanwhile attention should be called to the fact that by limit 
values in this connexion we must not understand the concentration 
y of the electrolyte added. From this a part is withdrawn by 
adsorption and hence, to the setting in end-condition appertains a 
lower concentration, which we will call x. In the experiments as 
to the current potentials we may probably identify the total con- 
centrations with the equilibrium concentrations as the adsorbing 
surface (the glass walls) is so small: only in the ease of the exceedingly 
weak AICI, solutions a doubt may arise. But in the colloid systems 
that difference may not be neglected. These y-values themselves 


Fig. 1.1) 


ae 
1) In Fig. 1 on the axis of coordinates should be read in stead of 
mm m 


626 
have been determined only for As,S,') and HgS, *) and for electro- 
lytes not used here. 

The proportions are : 

With As,S, XNH,Cl : XUO(NO;). —= 82 
» Hg,S ~xNH.Cl: XBaB, = 29. 

The proportion chosen 60:1 is, therefore, a rough approximation, 
but a comparison with y-values of other sols (P¢, Aw ete.) renders 
it probable that it represents the average. 

The relations between charge, adsorption and limit value are 
elucidated schematically in the above figure. In the upper half of 
the figure is drawn the charge ¢ of the capillary in dependence on 
the concentration of the traversing liquid, so that J, I], and III stand 
for uni-, di- and trivalent cations respectively. In the lower half is 
given, with the same concentration axis, the correlated adsorption 
of the electrolyte as a downward directed ordinate. If now y,, ¥%, 
and y, indicate the relation of the limit values for uni-, di- and 
trivalent cations, respectively the correlated downward directed ordinates 
must sbow the proportion 1:13 :3 and the upward directed ones 
equal values. 


4. For verification of this relation appeared suitable : 

(a) 10 uMol BaCl, — 600 uMol KCI. 

6) 25 uMol BaCl, — 1500 «Mol KCL. 

It would not do to simply take the specific conductivity powers 
as being proportional to the concentrations because in the so strongly 
diluted BaCl, solutions the conductivity power of water could not 
be neglected. Hence, I have made a direct measurement of the 
relation of the specific resistances by fillmge m1 Wuwatstonn’s bridge 
a vessel of arbitrary but fixed capacity with the liquids used. 

The relation of these resistances was in the pair (@) 

o, 4680 
— = —_—_=—19 
wk 247 

and in the pair (¢) 
oy 20 70n 
wr 99.9 


K , 
The values of P are obtained from the research communicated 
in the preceding paper. 


!) Freunpuicu, Zeitschr. f. physik. Chem. 73, 385 (1910). 
*) Freunpiicu en Scuucut, ibidem 85, 641 (1913). 


627 


As the relation of the potentials for (a) we obtain +4* or 14; as 
the relation of the resistances: 19. 


From the combination (4) we obtain for the potentials = cr 26, 
for the resistance 28. 

This agreement undoubtedly tells much in favour of the above 
mentioned theory. With concentrations somewhat larger than 60 the 


agreement might be better still. 


5. The material of Rifry') is only once suitable for testing the 
relation (2). 

For so far his measurements have been executed with solutions 
of salts other than chlorides his measuring electrodes were non- 
reversable ones and his results are therefore useless for quantitative 
verification. | have only been able to find one combination of 
chlorides where concentrations have been measured which are com- 
parable with limit values: they are KCl and HCl. For As,S,-sol 
these limit values have been determined to 50 and 31 mMol p. L. 
respectively °*). 

Now from his experiments Rifry has calculated the potential at 
the capillary wall in certain units for 0.01 n. KCl as 3.1. We can 
use this figure again for comparison purposes at it is directly propor- 
tional to the charge. 

In the case of HC] he determined for 0.005 7 : 3.39, for O.OLO 7 : 2.8, 
For the comparison with 0.01 2 HCl we must know the potential at 
the concentration #4 x 0.01 = 0.0062. This, | have interpolated by 
assuming that the logarithms of the potentials are directly propor- 
tional to those of the concentrations, after I had first convinced 
myself that this interpolation") formula was quite satisfactory in the 
longer series stated in Rigrys paper. We then find 3.2 which is 
again a splendid agreement. 


6. Quantitative comparisons with the trivalent cation are difficult 
to draw, because the y-values thereof are either not known or uncer- 
tain. From the treatises cited on p. 648 we, however, get the 
impression that the z-values diverge very little from zero, as is also 
expected from Table IV of the preceding communication, because a 
complete discharge takes place already at a concentration of 0.8 u mol. 


7. A no less striking parallelism between charge and limit value 

1) Ann. de chim. et de phys. [8], 30, 1 (1913). 

2) Frevuxpuicu, Kapillarchemie (Leipzig 1909) Table 81. True, those are 7- and 
not y-values, but with these univalent ions, this cannot have any serious influence, 

8) To this formula should only be attached the significance of an interpolation formula, 


41 


Proceedmes Royal Acad. Amsterdam. Vol, X VII 


628 


is furnished by the shape of the curve found for the current potential 
with AICI, solutions. This line is absolutely connected with the 
so-called irregular series. 

From what is stated in § 3 in connection with Table 1V (fig. 3, 
respectively) of the preceding paper it follows that the concentration 
at which the battery- shows an exchange of poles, is also that of 
the zero-charge of the capillary, whilst its positive charge goes up 
to about 3a mol. and thence lowers without however reaching zero 
again. An AICI, solution will consequently have first a discharging 
and therefore a coagulating effect on a negative sol. ; at higher concen- 
trations it will render it a positive sol and only at a much higher 
concentration it will again reverse the charge and cause coagulation. 
But therewith are described exactly the phenomena which, for instance, 
have been observed by Buxton and Taneur'), when they coagulated 
mastix with AICI, and indigo or Pt with FeCl,. The lower non- 
coalescent, the lower coalescent zone, the upper non- and coalescent 
zones, they can so to say be read off from the figures of the preceding 
communication. 

One is accustomed to attribute the phenomenon of the irregular 
series tO a special action of the hydrolytically resolved hydroxides 
of the coagulating ion. In connection with the preceding arises a doubt 
whether to Al(OH), ought really to be attributed a preponderating 
significance. For it does not seem probable that the AICI, which is 
present in such a small concentration, can cause a reversal of charge 
in the capillary. Much more acceptable seems the following idea. A 
strongly discharging cation unloads the capillary at such a small 
concentration that the small anion-concentration cannot prevent a 
complete reversal of charge. Of this the anion-concentrations are 
capable in the case of Ba and K- because there the charge gets 
nearer the zero value only at so much larger concentrations. 

Hence, the afterzone phenomenon will occur, as soon as the dis- 
charge by the cation is already very large at small concentrations— 
and is favoured by a feeble action of the anions. This strongly dis- 
charging action of the cation may arise from its higher valency or 
from its strong adsorbability. The fact that irregular series were 
observed, for instance, also with strychnine nitrate, new fuchsin, 
brilliant-green, auramine and_ silver nitrate *) is quite in harmony 
with this argument. For here we are dealing with strongly adsorb- 
able cations and because they are univalent the equivalent anion 

1) Z. f. physik. Chem. 57, 64 (1907. 

*) FREUNDLICH, I. ©. 


629 


concentration present is still proportionately three times less than 
with AICI,. 

A start has already been made with investigations to get a proper 
insight, particularly in this question of the irregular series. 


8. Finally it should be pointed out that the previous considera- 
tions also give an explanation of the fact often stated by us that in 
the ease of Al-salis we can determine the limit value much more 
accurately than with salts of uni- or bivalent metals. Two tubes with 
As,S, sol. which contain Al in concentrations situated 1°/, above 
and below the limit value, respectively exhibit after shaking a quite 
clear and a turbid fluid respectively. In the case of bivalent cations 
we must, so as to make quite sure, take the difference somewhat 
Jarger and very much so for a univalent ion. It is self-evident 

ae de 
that the cause lies in the fact that ae charge, ¢ concentration of 
coalescing ion) for Al is > for Ba and this again > for K-. 


Utrecht. June 1914. van ‘Tt Horr- Laboratory. 


{November 7, 1914). 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 
of Saturday October 31, 1914. 
Vou. XVII. 


Doce 


President: Prof. H. A. Lorentz. 
Secretary: Prof. P. Zeeman. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 3i October 1914, Dl. XXIID). 


ChE) ANF ah ao IN ae SS). 


G. van Rignsperk: “Jn the nerve-distribution in the trunk-dermatoma.” (Communicated 
by Prof. C. WinkixrR), p. 632. 

Ernst Couen and W,. D. Herperman: “The Allotropy of Cadmium” IV. p. 638. 

Ernst Conen and W. D. Herperman: “The Allotropy of Zine.” III, p. 641. 

Ernst Conen and J. C. van pen Bosco: “The Allotropy of Antimony”, I. p. 645. 

A. P. N. Francuimonr and H. J. Backer: “The Coloration of some derivatives of Pi- 
erylmethylamide with alkalies”. p. 647. 

A. P. N. Francutmonr and H. J. Backer: ‘“z-Sulpho-propionic acid and its resolution into 
optically active isomerides”’, p. 653. 

Miss H. J. Former: “A new electrometer, specially arranged for radio-active investigations.” 
Part I. (Communicated by Prof. H.-Iaca), p: 659. 

A. Suits: “The metastable continuation of the mixed crystal series of pseudo-components in 
connection with the phenomenon allotropy”. If. (Communicated by Prof. J. D. yan pER 
WaAats). p. 672. % 

A. Smits and S$. C. Boxnorst: “On the vapour pressure lines of the system phosphorus”. IT. 
(Communicated by Prof. J. D. van pER WaAALs), p. 678, 

A. Suits and A. H. W. Aten: “The application of the theory of allotropy to electro-motive 
equilibria.” III. (Communicated by Prof. J. D. van per Waats). p. 680. 

¥. E. C. Scurrrer: “On gas equilibria, and a test of Prof. van per Waats Jr.’s formula”, I. 
(Communicated by Prof. J. D. vAN per WaAAts), p. 695. 

W. Reivers: “Equilibria in the system Pb—S—O; the roasting reaction process”. (Commu- 
nicated by Prof. S. HooGrwerre), p. 703. 


Proceedings Royal Acad. Amsterdam, Vol. XVIL. 


632 


Physiology. — “On the nerve-distribution in the trunk-dermatoma’. 
By Prof. G. van Ruyperk. (Communicated by Prof. C. WINKLER). 


(Communicated in the meeting of September 26, 1914). 


We know as a result from the researches on the segmental skin- 
innervation, made after the method of the so called “remaining 
aesthesia’”’, first introduced by Snerrincton, that from a definite 
zone on the skin (the dermatoma or root-area) stimuli may reach 
the spinal cord along each separate dorsal root of the spinal cord. 
Such investigations, however, do not teach us anything about the 
manner in which the sensibility in each of these root-areas is 
provided for by the peripherical cutaneous nerves. A few experi- 
ments made on dogs have enabled me _ presently to offer the 
following conclusions concerning exclusively the dermatomata of 
the trunk. 

In a dissertation by O. NAnricn’), written under the direction of 
ELLENBERGER, the nerves providing the skin of the dog are described 
with elegant accuracy. It is shown therein, that the skin of the 


Fig. 1. Cutaneous nerves of the dog, according to NAuricu. —0O1 = Th. 1, first 
thoracic nerve, dorsal branch. rl = first thoracic nerve, lateral branch. rl = Th. 3, 
third thoracic nerve, ventral branch, ul = L. 1, first lumbar nerve, dorsal branch, 
q =nerve of the large subcutaneous muscle. 


1) O. N&uricw. Die Gefiihlshezirke und die motorischen Punkte des Hundes, 
Ein Beitrag zur vergl. Anatomie und Physiologie. Inaug. Diss. Ziirich 1907. 


633 


trunk is innervated by means of the perforating branches of the 
intercostal and lumbar nerves. 

If Th. 3 is taken to be the most cranial and L. 4 to be the most 
caudal nerve of the trunk, it will be found that from Th. 3 to 
Th. 7 each nerve-root is sending three perforating branches to the 
skin: a dorsal, a lateral, and a ventral branch. The dorsal nerve- 
trunk generally supplies two main branches: a medio-dorsal and a 
dorso-lateral one. The lateral nerve invariably supplies two branches : 
a latero-dorsal and a latero-ventral branch. The ventral nerve-trunk 
usually consists of one main trunk, which may be said to be medio- 
ventral. From Th. 8 to L. 4 the medio-ventral branches are wanting: 
their place is taken by the latero-ventral ones. 

The different points, where the dorsal, lateral, and ventral nerves 
enter into the skin, may be interconnected by lines. This having 
been done, it becomes evident that the dorsal branches, going in 
a cranial-caudalward direction, perforate the fascia continually at 
a greater distance from the mid-dorsal line, whilst the lateral trunks 
on the contrary come forth more dorsalward. A correct insight into 
the relations of these nerves is offered by Fig. 1. From Fig. 2 it 
may be seen moreover, that the skin of the trunk can be divided, 
according to a superficial scheme, into three zones as regards its 
peripherical nerves: a dorsal, a lateral, and a ventral zone. 


rt dyrsales dM 
yok 
Framt laterales dda tntercostalest > 


. cum M pectoralts dorsaltsve 
} Ss Ash 


> 
Ss 
J 
Q 
nn 
S 
& 
JA & 
ast! > 


=~ 


~ Netut hunger pest W axill) 


B . cul cruris 


_ anterior, 
Se 


Fig. 2 Extension-zones of the dorsal, lateral, and ventral nerve-branches of the 
skin of dogs, according to NAuricu. 


I. The first question I now put to myself was the following: are 
the perforating dorsal, lateral, and ventral trunks, which belong when 
42* 


634 


prepared macroscopically, to one intercostal resp. to one lumbar 
nerve, unisegmental or pluri-segmental nerve-canals. For whilst it 
is admitted almost generally that the intercostal nerves are uniseg- 
mental courses, Ersier') believes “he has sufficient grounds for 
stating that delicate nerve-plexus, situated on the inside of the ribs 
always connect two intercostal nerves. This being so, an interchange 
would oceur here between nerve-fibres of a different segmental origin. 
Concerning the nerve-distribution of the root-areas, this question 
may be formulated as follows: Do the nerve-fibres of each separate 
dorsal root of the spinal cord reach the skin-area belonging to that 
root along one single dorsal lateral or ventral perforating nerve- 
trunk, or along several ones? 

In order to solve this question, I made the following experiment. 
After the afore mentioned method of Samrrinctron, the dorsal (and 
ventral) spinal nerve root of a segment on one side of the spinal cord 
of some dogs was “isolated”, usually between three cranial and as 
many caudal roots, which were cut through extradural. This being done, 
the isolated root-area, corresponding to the isolated root, was 
demareated against the two insensible zones, corresponding to the 
sectioned roots. Situation, form and extension of the sensible root- 
area once being well defined, the skin was entirely cleft both in the 
cranial and in the caudal insensible zone by a slit passing from 
the mid-dorsal to the mid-ventral line. This of course could be done 
without narcosis. Immediately after this, a search was made for 
the perforating skin-nerves, and at least three successive ones of 
these in cranio-caudal direction, in the dorsal, lateral, and ventral 
skin-area, were prepared free, as much as possible avoiding any 
lesion of them. Next to this, by means of the induction-current, 
these nerves were stimulated to ascertain whether they conducted 
painstimuli. Invariably the result was, that for each skin-area such 
was only the case with these branches that belonged to one point 
of entrance. lrritation of the other branches, even with the strongest 
induction currents (the bobbin being entirely pushed in), never 
produced any symptom of pain, if slippings of the current were 
avoided. This result was wholly confirmed by a contra-experiment. 
If, after careful determination of the dorsal, lateral and eventually 
ventral branches, which were conductors of pain-stimuli, these branches 
were cut through, the sensibility in the isolated root-area proved to 
be destroyed entirely and irrevocably. 


1) P. Etster. Ueber die Ursachen der Gefleclitbildung an den peripheren Nerven. 
Verh. d Anatom. Gesellsch a. d. 16e Vers. in Halle. 1902. S. 200. 


635 


Thus it results that the trunk-skin of the dog forwards its stimuli, 
destined for a definite segment of the spinal cord, only by means 
of one set of peripherical skin-nerves. This means that in those 
nerves only fibres belonging to one posterior root have their course, 
and that consequently the perforating skin-branches are segmental 
nerve-canals. 

II. A second question, necessarily presenting itself, is the following 
one: what separate portion within the dermatoma is innervated by 
either the dorsal or the lateral (ventral) peripherical branches ? 

To investigate this, the above-mentioned method was partially repeated 
once more. With dogs, where a nerve-root had been isolated, the 
peripherical branches entertaining its sensibility were sought for and 
prepared free. After this the conduction was successively interrupted, 
either provisorily or lastingly, in one or more of these branches. 
To obtain a lasting interruption of the conduction, the branch was cut 
through. For a provisory interruption the branch was enfolded by a 
piece of cottonwool, drenched in a 5°/, solution of stovaine. The 
conduction .once interrupted, the root-area was tested to ascertain 
whether a portion of it had become insensible, and if so the confines 
of the insensible area found in this manner were determinated. 


Fig. 3. On a dog a root-area (Th. 10) has been isolated between two 
insensible zones. After this, three cutaneous branches belonging to the dorsal 
perforating nerve-trunk, are successively cut through. The dotted portion 
of the root-area then becomes successively insensible, until finally the whole of 
its dorsal part has lost sensibility. 


a. Interruption of the conduction in the joint dorsal cutaneous 
branches. 


636 


After this operation the entire dorsal portion of the isolated 
dermatoma was found to have lost sensibility. To make the ventral 
demarcation of the area that has been made insensible in this way 
rightly understood, I may add the following: For a long time I had 
been struck by the fact that after a carefully performed root-isolation, 
the demarcation-lines of the isolated root-areas showed at a definite 
point a distinct bent. The origin of this bent is, that at some 
distance from the mid-dorsal line of the body, both the cranial 
and the caudal demarcation lines of the root-area, change their 
direction somewhat cranialward. In the cranial demarcationline this 
bent is always found a little more dorsalward than in the caudal 
demareationline. Now it is remarkable, that the ventral limit of the 
insensible zone, originated by the sectioning of the dorsal nerve- 
branches, is invariably found to be a straight line, connecting the 
cranial with the caudal limit just above this bent. This line therefore 
goes in a cranio-caudal direction. At the same time however it 
deviates slightly in a dorso-ventral direction. Consequently the 
latero-ventral nerves supply within the root-area the innervation of 
a zone extending to a point somewhat above the alleged bent in 
its demarcation-lines. 

6. If the conduction is interrupted in the joint latero-ventral 
branches, the entire ventral portion of the root-area becomes insensible. 


Fig. 4. The same as in ig. 3, only for branches of the Jatero- 
ventral trunk. (The isolated root-area is probably in the main Th. 12. 
Its closer definition was neglected in the necropy.) 


If we compare the demarcationline found in this way, with that 
found after interrupting the conduction in the dorsal branches, it 
becomes evident that the ventral boundary of the dorsal area does 


not coincide exactly with the dorsal boundary of the ventral area, 
but that a reciprocal overlapping occurs, although it be only a 
slight one. It is shown thereby that the bent, found in the demar- 
cationline of the root-area, is situated exactly at the point where the 
dorsal and latero-ventral portions of the dermatoma meet. The cranial 
direction of this bent indicates that the latero-ventral portion must 
be lying somewhat more cranialward than the dorsal one. This fact 
has been stated previously by Bok"), when he found in 1897 a 
“discrepancy” of the dorsal and ventral dermatoma-areas on the 
human trunk. In the experimentally defined dermatoma this discre- 
pancy finds its expression in the alleged ‘bent’. Similar conditions 
have been observed clinically by Eicuuorst’), after transversal lesions 
of the spinal cord in the trunk-area. 

ce. Interruption of the conduction in separate minor branches of the 
dorsal and Jatero-ventral nerves. 

The conduction may be interrupted in the separate minor branches 

of the perforating nerves as well in the dorsal as in the latero-ventral 
portion of the root-area. When this operation has been performed it 
becomes evident, as long as only the larger branches were subjected 
to it, that each of these supplies the innervation of a small zone, 
extending equally into the cranial and into the caudal boundary of 
the root-area, and for the rest demarcated by lines going in a 
cranio-caudal direction. The whole root-area therefore is divided 
into a series of small areas, lying alongside of one another in 
dorso-ventral direction. The skin-area of the medio-dorsal branch 
adjoins the mid-dorsal line, the dorso-lateral branch on the other 
hand extends over an area, adjacent to the lateral portion of the 
dermatoma, more ventralward than that of the medio-dorsal branch. 
A similar ordination is found likewise to exist for all skin-areas 
corresponding to the various latero-ventral branches. 
Whenever very thin branches are cut through, either no insensi- 
bility ensues, or else an irregularly insensible spot is found some- 
where within the root-area. From the fact that in many cases, after 
the sectioning of such small branches, no insensibility is found, we 
may conclude that the areas of extension of the separate branches 
of the cutaneous nerves must overlap one another to a certain degree. 
I have not been able however to determine the extension of these 
overlappings. 

1) L. Bouk, A few data from the segmental anatomy of the human body. 
Ned. Tijdschrift v. Geneeskunde. 1897. I p. 982—995, and 1897. II. p. 865—379. 
(Compare especially p. 366 et seq.). 

2) H. ErcHaorsr, Verbreitungsweise der Hautnerven beim Menschen. Zeitschr. 


f. Klin. Medicin. Bd. XIV. S. 519. Berlin 1888. 


638 


Ill. Finally my attention was given to the nerve of the subcutaneous 
muscle. NAnricn') testifies that by irritation of this nerve, in addition to 
contraction of the cutaneous muscle, also pain-symptoms are brought 
forth, whilst after the sectioning of this nerve, the sensibility of the 
skin had diminished. I have not been able to verify this latter fact. It 
is not to be doubted moreover that e.q. an isolated root-area, if either 
the isolated root or the peripherical branches have been cut through, 
becomes entirely and completely insensible, whilst the nerve of the 
cutaneous muscle remains intact. It is therefore probable that this 
nerve does not contribute to the sensibility of the skin. Nevertheless 
I can confirm the statement of NAurica, that after its having been 
cut through, irritation of the central end proves painful. It may be 
that the muscular sensibility plays a part in producing these symp- 
toms of pain. 


Chemistry. — “The Allotrepy of Cadmium.” 1V. By Prof. Ernst 
Courn and W. D. Her.peErMAn. 


(Communicated in the meeting of September 26, 1914). 


The electromotive behaviour of Cadmium. LI. 


1. Up to the present we have only directed attention to the 
electromotive behaviour of @- and y-cadmium; the 8-modification has 
not been mentioned hitherto. It will be treated in the following lines. 

2. It may be remembered that a number of cells constructed 
according to the scheme: 

Cd Guinea | Cd-amalgam 
electrolytically : fee 12.5 percent 
cenosied cadmium sulphate | py een 
had an E.M.F. of 0.050 Volt at 25°.0, whilst the E.M.F. of others 
was only 0.047 Volt at the same temperature. (The cells were 
reproducible within 0.5 millivolt). 

3. Now we were struck by the fact that when constructing a 
large nuniber of these cells we often got cells which had an E.M.F. 
of 0.048 Volt at 25°.0. 

The E.M.F. of cells which originally had an E.M.F. of 0.050 Volt 
at 25°.0, spontaneously decreased till the value 0,048 Volt was reached. 
After this their E.M.F. remained constant. 

4. The conclusion was plain that the cells giving 0.048 Volt might 


1) L. c. p. 95—96, 


639 


contain /-cadmium, those giving 0.047 Volt ecadmium, whilst those 
giving 0.050 Volt have y-cadmium as a negative electrode. 

5. If this were really the case, it would be possible to construct 
a transition cell by combining a cell with a@-cadmium with one 
containing B-cadmium,; the E.M.F. of this combination would be zero 
at the transition temperature of the change v-cadmium 2 p-cadmium. 

6. However it is impossible to carry out an exact determination 
of the transition point in this way, as the E.M.F. of the combination 
is (at 25°.0) only (0.048—0.047) = 0.001 Volt and the reproducibility 
of each of the cells is only 0.5 millivolt. 

7. In order to ascertain if the E.M.F. of the B-cells has a real 
significance, experiinents may be carried out on the following lines: 

At temperatures above the transition point of the change «-cad- 
mium 2 #-cadmium (which we found in the neighbourhood of 60° 
by dilatometriec measurements) the E.M.F. of a@-cells must be higher 
than that of p-cells. After cooling the cells below the transition point 
mentioned, the contrary will occur. 

8. Our experiments in this direction were carried out in the 
following way: 

We constructed a large number of Hurnrr cells’); one of these, 
the E.M.F. of which had been originally 0.050 Volt at 25°.0, had 
an E.M.F. of 0.047 Volt (at 25°.0) after having been kept for 4 weeks 
at 47°.5. After this time it remained constant. 

We combined this cell (N°. 7) with 
another one (N°. 22) the E.M.F. of 
which was 0.048 Volt at 25°.0. The 
two cells AB (N°. 7) and CD (N°. 22) 
were connected by a siphon H, 
which contained the same solution 
of cadmium sulphate as was present 
in the cells. (Fig. 1). 

The lateral tube E of the siphon 
was closed by a rubber tube F, in 


which was put a glass rod G. The 


little apparatus was brought into a 
Fig. 1. thermostat which could be kept at 

will at 25°.0 or 64°.5. 
9. We measured the E.M.F. between the cadmium which had 
been electrolytically deposited on the platinum spirals A and C 


1) Proceedings 17, 122 (1914), 


640 


against the common amalgam electrode B. (12.5°/, by weight). It 
is absolutely necessary to use a common electrode as the cadmium 
amalgam of 12.5 percent by weight does not form a heterogeneous 
system at 64°.5; its E.M.F. is then a function of its composition. The 
use of the #vo amalgam electrodes B and D might give rise to 
serious mistakes, if there were only small differences in their com- 
position. 

The absolute E.M.F. of our amalgam electrode against cadmium 
in A and C does not play any role in our measurements. 

10. The determinations of E.M.F. were carried out by the Poe- 
GENDORFF compensation method. The resistances used, had been checked 
by the Physikalisch-Technische Reichsanstalt at Charlottenburg— 
Berlin. The same was the case with the thermometers used. Our 
two standard elements (WesToN) were put into a thermostat which 
was kept at 25°.0. We used as a zero instrument a Deprez-D’ ARSONVAL 
galvanometer, which was mounted on a vibration-free suspension 
(Junius). The readings were made by means of a telescope and scale; 
0.02 millivolt could easily be measured. 

The determinations were continued during several days, until the 
E.M.F. of the cells had become constant. 

Our table I shows the results. 


GAs elves ale 


Temperature 25°.0. 
E.M.F. 
Cell 7 0.04741 Volt 
Cell 22 0.04815 _,, 


Temperature 64°.5 


Cell 7 0.04029 Volt. 
Cell 22 0.03979 __,, 


After having brought the cells to 25°.0, we found: 
Celli 0.04741 Volt. 
Cell 22 0.04806 __,, 


The table shows that at 64°.5 there has taken place an inversion 
of the poles and that the cells regain their original E.M.F. at 25°.0. 

A second experiment with two cells (n°. 4 and 8) newly con- 
structed, gave the following results: 


641 


AM Nasa a8 JN 


Temperature 25°.0, 
E.K. 
Cell 8 0.04757 Volt 
Cell 4 0.04839 _,, 


Temperature 64°.5. 
Cell 8 0.04737 Volt 
Cell 4 0.04633 _,, 


After having brought the cells to 25°.0, we found: 
Cell 8 0.04776 Volt 
Cell 4 0.04789, . 

11. From table II it may be seen that we are here at the limit 
of measurement obtainable in working with cells of so small an 
E.M.F. the reproducibility of which is 0.5 Millivolt. 

12. From the inversion of poles which has been observed, we 
may conclude that the value 0.048 Volt at 25°.0 really has signi- 
licance and is to be attributed to the presence of $-cadmium. 

13. As to the bearing of the existence of different modifications 
of cadmium on the E.M.F. of the standard cell of Weston, we 
refer to our paper “On the Thermodynamics of standard cells” 
(sixth communication), published some months ago '). 

Utrecht, September 1914. van “Tt Horr- Laboratory. 


Chemistry. — “The Allotropy of Zinc.” I. By Prof. Ernst 
Couen and W. D. HeLperMan. 
(Communicated in the meeting of September 26, 1914). 


1. In our first communication on the allotropy of zine’), we 
summarized the earlier literature on this subject as follows: as long 
as half a century ago various investigators tried to solve the problem 
whether zine might be capable of existing in different allotropic 
modifications. As late as 1890 Le Cratetimr proved that this metal 
does really show a transition point in the neighbourhood of 350°. 
Monkemerer found this point at 321°, Brnepicks at 330° (melting 
point of pure zine 419.°4) whilst the measurements of Max Werner 


i 1) Chemisch Weekblad 11, 740 (1914). This paper will be published before long 
in the Zeitschr. f. physik. Chemie. 
2) Proceedings 16, 565 (1913). 


642 


(who found 800°), published some weeks ago, agree sufficiently with 
those of Le Cuarruimr. We shall discuss in a subsequent paper the 
differences which exist amongst the results of the investigators mentioned 
above. Whilst Brenepicks mentions a second transition point (at 170°), 
Max Werner was unable to find this point. The question as to 
whether it really exists or not, may be left open for the moment. 

2. Since writing the above we became acquainted with the paper 
of Le Verrier’), which has been summarized by one of us’). 
Le Verrter found that the specific heat of zine varies greatly between 
100 and 140° and that there oceurs an absorption of heat within 
this interval of temperature of O—8 calories. This result indicates 
that there exists here a transition point. Mr. G. pe Bruin is carrying 
out a systematic investigation in this direction. 

3. Brnepicks and RaGnar Arpt have recently published *) a new 
investigation of this subject. In his first paper BrnEpicks pointed out 
that ‘‘beziiglich der Frage, ob die fiir das Zine. puriss. Merck 
(garantiert frei von Kisen und Arsen in Staben) gefundenen Angaben 
auch fiir das absolut reine Metall gelten, bedarf es ebenfalls weiterer 
Versuche”’. 

That there was no reason to suppose that this sample contained 
impurities may be coneluded from the authors’ words: “Jedoch ist 
es im Hinblick auf die Wichtigkeit der Reinheit dieses Produktes 
fiir seine Verwendung fiir analytische Zwecke sehr wahrscheinlich, 
dass die Menge von Fremdkérpern zu vernachlassigen ist’. 

4. However Brnepicks writes in his most recent paper: “Es ist 
deshalb hier eine Revision der einschlagigen Verhaltnisse vorgenomen 
worden, die zu ziemlich unerwarteten Ergebnissen gefiihrt hat. Namlich, 
dass iiberhaupt keine Allotropiebeweise fiir Zink z. Z. vorliegen”. 
He adds: “ Abgesehen wird dabei zuniachst von derjenigen Andeutung 
von Allotropie, die neuerdings von EK. Courn und W. D. HeLpEermMan 
durch spez. Gewichtsbestimmungen gefunden wurde”. We shall 
revert to this point later. 

5. The method followed by Brnepicks and Arpi to discover 
possible transition points was the same as used formerly by BEnepicks, 
viz. the determination of the electrical conductivity of the metal at 
different temperatures. 

Whilst he found in his first determinations (working with zine. 
puriss. Merck) transition points at 170° and 330° respectively, he 
was not able to find them when he used ‘Zine KaHLBaum”’ which 


i) C. R. 114, 907 (1892). 
2) Ernst Conen, Proceedings 17, 200 (1914). 
5) Zeitschr. f. anorg. Chemie 88, 237 (1914). 


643 


only contained 0,0047°/, of Cd., 0,0033°/, of Pb., 0,00045°/, Ke,Cu). 

But working with the same material to which 0.52 per cent by 
weight of Cd, resp. 0,5 per cent of Pb. or 0,5 per cent of Cd--0,5 
per cent of Pb had been added, he found several transition points 
which grosso modo agreed with those found formerly by Brnapicks a.o. 
On account of these results Benrpicks and Arvr conclude that the 
transition points found by Brnepicks in his first investigation are to 
be attributed to impurities in the metal used and that zine which 
is pure does nof show transition points. 


6. In the first place it may be pointed out that the curves which 
form the basis of the authors’ conclusions, are so roughly defined, 
that it is almost impossible to conclude anything from them. For 
example, from a consideration of the curve 2 in Fig. 2 (which refers 
to pure zinc), one might arrive at the conclusion that a break ') 
exists at 150°. 


7. However, a more serious objection to the method followed, 
may be pointed out. Our recent investigations on the allotropy of 
metals have shown that the changes in these substances take place 
very slowly even at high temperatures. These retardations can only 
be removed by special means (inoculating in contact with an electro- 
lyte, repeated changes of temperature etc.). We may call to mind the 
fact that we were able to heat cadmium 95 degrees above one of 
its transition points without any changes occurring. It will be necessary 
to give special attention in future to these phenomena, which play 
also a role in ‘thermal analysis” and which may falsify its results. 

Benepicks and Arpr did not make any provision to eliminate these 
phenomena. On account of what we know now about these hyste- 
resis phenomena it was to be expected that any transition point, if 
it really existed, would only be found under favourable circumstances, 
or by a systematic elimination of the retardations mentioned above. 


8. Moreover it may be pointed out that Benepicks and Arpt made 
the supposition “dass die betreffenden Metalle nicht geniigend rein 
waren” (viz. the zinc. puriss. Merck, used by Brnepicks in his first 
investigations and by Le Caaretier among others). We think that the 
opinion put forward by Brnepicks in his first paper (see above § 3) “dass 
die Menge von Fremdk6rpern zu vernachlassigen ist’’, is the just one. 
As we were told by Messrs. Merck at Darmstadt their ‘Zinc. puriss. 
Merck (garantiert frei von Hisen und Arsen in Stiben)” contains only 
small traces of cadmium. We carried out an analysis of this material 


‘) Whether this point really exists or not may be left open for the moment. 


644 


following the method described by Myzius?). In 100 gr. of this metal 
we could only detect small traces of cadmium (lead and iron). We 
think that the explanation of B. and A. which is based on the 
presence of large amounts of impurities falls to the ground. 


9. That it is not the presence of foreign substances which give 
rise. to the strongly marked change of the mechanical properties of 
zine at higher temperatures (which fact has been the starting point 
of Brnepicks’ investigations) is evident from the fact, that this change 
may also be observed in the purest zine (Zink ‘Kahlbaum”, comp. 
§ 5). We bave been able to confirm this result repeatedly ourselves. 


10. Finally some remarks, made in a note by Bengpicks and ArpI 
may be considered here. 

In the first place they believe, on account of an investigation con- 
cerning the quenching velocities of metals, carried out by BENEDICKs *), 
that “eine besonders grosse Abkiihlungsgeschwindigkeit nicht zu erzielen 
ist” when the method is followed which we used. (1 kilo of zine 
was chilled in a mixture of solid carbid dioxide and alcohol). It 
may be pointed out that the velocity we used has been greatly exag- 
gerated; we got the same results by using water or air of room tempe- 
rature. We also carried out some experiments with carbon dioxide 
and aleo hol in order to vary the external conditions of our experiments 
as much as possible. In our researches on the allotropy of copper 
and cadmium we also used water or air as a cooling medium. 


14. Secondly Benwpicks and Arpr raise the question as to whether 
there has not taken place an ‘Auflockerung der Oberflache” of our 
preparations when we washed them with dilute hydrochloric acid. 
By this operation a change of density might have occurred. 

They have however overlooked two facts: in the first place the 
recent investigations of JouHnsron and Apams*), which prove that the 
density of any substance is independent of its state of division. 
Moreover they have not taken into account the results of our inves- 
tigations on cadmium‘), where the same difficulties would have 
occurred. The reproducibility and reversibility of the phenomena 
prove that the disturbances, mentioned by BrNepicks and Arpi really 
do not occur. 

We hope to report shortly on the real transition points of zine. 

Utrecht, September 1914. van “t Horr-Laboratory. 

1) Zeitschr. f. anorg. Chemie 9, 144 (1895); Myxius, ibid. 74, 407 (1912). 

2) Journ. of the Iron and Steel Institute 77, 153 (1908). 


3) Journ. Americ. Chem. Soc. 34, 563 (1912). 
4) Proceedings 16, 485 (1913). 


645 


Chemistry. — “The Allotropy of Antimony.” I. By Prof. Erxst 
Conen and J. C. van pen Boscn. 


(Communicated in the meeting of September 26, 1914). 


1. The following modifications of this metal were known hitherto: 

a. The so called metallic antimony, a bluish-white solid with 
metallic lustre. It is very brittle at ordinary temperatures and is 
said to crystallize in the hexagonal system. Only this modification 
is found in nature. 

6. Black antimony. This form has been prepared by Stock and 
Siebert’) in three different ways, the best method being by rapid 
cooling of the vapour of ordinary metallic antimony. This black 
modification is converted by heating into metallic antimony. Its colour 
and density change slowly at 100°; at 400° the conversion occurs 
instantly. This form seems to be metastable at ordinary temperatures. 

c. Yellow antimony was first prepared by Stock and Gu?TTMANN *) 
in the year 1904, by the interaction of antimony hydride (at —90°) 
with air, oxygen or chlorine. Even at — 50° this form is meta- 
stabie: it is converted by heating into the black modification. 

d. Explosive Antimony. Ernst Conrn, Rinckr, StRENGgRs, and 
Cotuins*) proved that the explosion which occurs when this body 
is pounded, pressed or scraped, is to be attributed to the transformation 
of an allotropic form called by them 3-antimony, into the ordinary 
modification (metallic antimony ; ¢-antimony). Hitherto no investigation 
of the connexion between these different forms has been carried out 
as it is very difficult to procure sufficiently large quantities of them. 

2. The investigations described below deal with the question 
whether the metal known hitherto as “metallic antimony” is to be 
considered at ordinary temperatures and pressures as a metastable 
system, as is the case with the metals we have already investigated. 
Our experiments will prove that this is really the case. 

3. A kilogram of antimony (KaniBaum — Berlin) which contained 
some hundredths of a percent of impurity, was melted and poured 
into a cylinder of asbestos paper, which was surrounded by a mixture 
of aleobol and solid carbon dioxide. The chilled metal so obtained 
was used in all experiments. 

4. It was powdered in a mortar. We determined its density at 
25°.0 using two pycnometers as described by JoHNnsron and Apams‘), 


1) Ber. d. d. chem. Ges. 38, 3837 (1906). 

2) Ber. d. d. chem. Ges. 37, 885 (1904). 

8) Zeitschr. f. physik. Chemie 47, 1 (1904); 50, 292 (1904); 52, 129 (1905). 
4) Journ. Am. Chem. Soc. 34, 563 (1912). 


646 


The difference between any two of these determinations never exceeded 
three units in the third decimal place. 
Our thermometers had been compared with a standard of the 


Phys. Techn. Reichanstalt at Charlottenburg — Berlin. 
We used toluene as the liquid in the pyenometer; its density had 
KO 


fe a0. ad 
been determined in four experiments to be d =e, 0.8603. 


Two different parts (A) and (/) of our material gave the values 
25°.0 6.6900 (A) and 
4° 6.6897 (£). 

5. The samples (A) and (2) were now heated separately during 4 x 24 
hours in an aqueous solution of potassium chloride (10 gr. KCI on 
100 er. of water), using a reflux condenser, the boiling point of the 
solution being 102°.5. 

The metal was then washed with dilute hydrochloric acid, water, 
aleohol and ether, and dried iz vacuo over sulphuric acid. 

Its density was now 
25°.0 6.6744 (A) 
4° 6.6803 (E); 

Consequently the density has decreased by 13 units in the third 


ad. 


decimal place. 

6. After having heated (A) and (/) for a second time (6 x 24 

hours) in the boiling solution, we found: 

25°.0 6.6784 and 6.6765 (A) 
“4° «6.6789 and 6.6778 (E). 
The density had undergone no further change. 
7. The experiments described in §§ 4—6 show that the antimony 
after chilling is present in a form which changes at 100° with a 
measurable velocity. 

In order to investigate if there exists here a transition tempera- 
ture as in the case of the other metals which we have hitherto 
studied, we carried out some dilatometric measurements, using the 
electric thermostat which we described formerly. *) 

8. The material which was put into the dilatometer consisted of 
small pieces of the metal mixed up with fine powder and a part of 
the metal from the pyenometers. (500 grams). The paraffin oil used 
had been heated for some time at 200° in contact with finely divided 
antimony. There was no evolution of gasbubbles. 

9. At temperatures below 119° there occurred no change of the 
meniscus at the jirst heating (the bore of the capillary tube was 


1) Zeitschr. f, physik. Chemie 87, 409 (1914). 


647 


1 mm.), not even when the heating was continued for 48 hours. 

On the contrary, the dilatometer having been kept at 15° during 
a month, the change was: 

At 101°.8 in 2 hours, + 74 mm.; ie. + 37 mm. per hour 

a OO ORR Te Ar so> = 20, oe ells A Re ac 

NOON el 5 BO Pre ala ha ae, 

From these data one might conclude that there exists a transition 
point in the neighbourhood of 101° which is in perfect agreement 
with our density determinations (§ 4—6). 

10. Guided by the experience gained in the case of cadmium and 
copper‘), we now earried out some experiments with antimony 
whose previous thermal history had been changed between wide limits. 

After having kept the dilatometer for 50 minutes at.150°, the 
meniscus fell during a certain time at the constant temperature of 
96°.0; after this it became stationary and then began to rise. From 
these observations one would conclude that there is a transition 
point below 96°.0 and that, in consequence of the heating at 150°, 
the transition temperature had thus been lowered. This experiment 
proves, that at 96°.0 there are present at the same time more than 
two modifications. 

11. The dilatometer was now kept at 225° for 12 hours. After 
this there occurred at 94°.6 (at constant temperature) a marked fall 
in the oil level (569 mm. within 48 hours), while in the experiment 
described in § 10 there took place a rise of the meniscus at the 
same temperature. 

12. The phenomena deseribed above show that meta/lic antimony, 
such as we have known it hitherto, is also a metastable system 
which consists of more than two allotropic forms. 

We hope shortly to report on the modifications which play a 
role here. 

Utrecht, April 1914. van ‘t Horr-Laboratory. 


Chemistry. — “Vhe Coloration of some derivatives of Picrylne- 
thylamide with alkalies’. By Prof. A. P. N. Francumonr and 
H. J. Backrr. 
(Communicated in the meeting of September 26, 1914). 

In a previous communication (Fee. trav. chim. 1913, 82, 325 ; Abstr. 
Chem. Soc. 1914, ii, 84) we described the spectrographie investigation 
of the coloration which picrylalkylnitramines undergo by alkalies. It 
was shown, that the absorption spectrum of picrylmethylnitraimine 
C,H, (NO,), N Me(NO,) after addition of alkali gets a certain ana- 


1) Proceedings 17, 54, 60 (1914). 


43 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


648 


logy with that of picrylmethylamide C,H, (NO,), NHMe, and that the 
latter spectrum is not much changed by alkali. 

We then concluded, that the coloration of picrylalkyInitramines 
with alkalies had a similar cause as the colour of nitranilines (wid. 
Francumont, Rec. trav. chim. 1910, 29, 298, 313), which is ascribed 
by Hanrzscu (Ler. 1910, 48, 1669) to an action between the nitro 
and amino groups attached to the benzene nucleus. The coloration 
of the nitramines would thus be produced by nitro groups of the 
nucleus reacting with the base, the nitro group attached to nitrogen 
playing only a secondary part. 

In order to test this hypothesis, we have now examined several 
derivatives of picrylmethylamide, compounds of the formula Pier. 
N Me X?). For X we have chosen the nitroso group, the organic . 
acyl groups COCH,, CO,Me, CO,,Et and finally the phenyl group 
as example of a negative group being no acylgroup. The compounds 
investigated were thus picrylmethyInitrosamine Picr. N Me(NO), pieryl- 
methylacetamide Picr. NMe(COCH,), methylpicrylmethylaminoformiate 
Picr. N Me (CO,Me) and the ethylester Picr. NMe (CO, Et), and picryl- 
phenylmethylamide Pier. NMe Ph. 


In the first place it should be observed that, like the nitrogroup, 
also the acyl groups NO, COCH,, CO,Me, CO,Et strongly diminish 
the colour of the picrylmethylamide. Compared with this deeply 
yellow coloured amide, the nitramine, nitrosamine, acetyl derivative 
and both the urethanes are only palish yellow. 

These differences are clearly shown by the absorption curves. 
Both the absorption bands of pierylmethylamide at = 2390 and 2875 
(see curve 15) disappear wholly; the acyl derivatives give for the 
concentrations examined, only a continuous absorption in the ultra- 
violet (curves 3, 5, 8, 10), just as it was found for the nitramine 
(Rec. trav. chim. 1913, 32, 332). 

It must be admitted, that the presence of acyl groups in the 
aminogroup of picrylmethylamide so strongly diminishes the basie 
properties of this group, that it loses the power to act with a nitro- 
group, and thus to produce colour. 

If this hypothesis is correct, it must be possible to prevent this 
reaction also by addition of a strong acid combining witlr the 
amine group. 

Indeed, picrylmethylamide dissolves perfectly colourless in strong 


1) In this paper Pier. means the group 2, 4, 6-trinitrophenyl. 


649 


sulphurie acid. The absorption bands disappear wholly from the spec- 
trum, and only a modest continuous absorption in the ultraviolet remains 
(compare curves 14 and 15). For a concentration of 0.0002 gram- 
molecules per litre and an absorbing layer of 100 m.m. the beginning 


il 
of the absorption is repelled by the sulphuric acid from  — 2150 to 


3400. This decoloration of picrylmethylamide by sulphuric acid is 
just the reverse of the coloration of the nitramine with alkali. In 
the first case the nitro groups of the nucleus are deprived of the 
opportunity to combine with a basic group, in the latter case this 
opportunity is on the contrary given. 


The reaction with alkalies seems to be the same for the acylderi- 
vatives now investigated as for the pierylalkylnitramines, the only 
difference being that they want a little more alkali for the red 

mY 


coloration. Formerly we found (Rec. trav. chim. 1918, 32, 332), 
that a solution of picrylmethylnitramine containing an excess of 


1 
alkali gives two bands at A 1975 and 2350. At nearly the same 


places two bands are shown by the alkaline solutions of the acetyl 
derivative (curve 6) and the urethanes (9 and 11), though one of 
the bands is only represented by a flat part of the absorption curve. 

The anomalous curve given by the nitrosamine with alkali (4) 
will be discussed separately. 

Pierylphenylmethylamide, the last derivative of picrylmethylamide 
we examined, exists in two forms of the same dark red colour but 
of different melting points, 108 and 129°. Hanrzscu (Ber. 1910, 98, 
1651) calls the two forms homochromo isomerides, whilst BitMANn 
(Ber. 1911, 44, 827) regards them as polymorphous forms. 

As Hawnrzscu has already observed, the spectra of the two forms 
are completely eqaal (curve 12). It was now found, that the «and 8 
forms in presence of alkalies also behave in the same way (curve 13), 
so that the two forms when dissolved seem to be wholly identical. 
The broad absorption band of the amide at 2350 becomes by addition 
of alkali a little deeper and is somewhat displaced to larger wave- 
lengths. At the same time it undergoes a division into a flat part at 
2070 and a feeble band at 2400. This agrees with the behaviour 
of the other compounds with bases. 

Finally we have examined the coloration of 1,3,5-trinitrobenzene 
with alkali, since here only the nitrogroups of the nucleus can act 
with the base. 

Whilst trinitrobenzene only absorbs continuously (curve 1), addition 

43% 


650 


of alkali produces a broad band from 2040 to 2300 (curve 2). Its 
centre is at about the same place as the centre of the two bands, 
which show the picrylmethylamide derivates in presence of alkalies. 


In the previous publication (l.c.) we mentioned a remarkable 
decomposition of the alkaline solution of picrylmethylnitramine. After 
a day it gave the spectrum of potassium picrate, being hydrolysed in 
this way: Pier. N Me NO, — Picr. OH + Me NH NO,. 

An analogous decomposition takes place, though more slowly, with 
the acetyl derivative and the two urethanes. In a few days the spec- 
trum of their alkaline solutions is perfectly the same as that shown 
by potassium picrate (curve 7). 

With picrylmethylnitrosamine this decomposition proceeds very 
quickly, much more rapidly than with the nitramine. During the few 
minutes required for the spectrographic examination its alkaline 
solution is already partly decomposed. ; 

The anomalous absorption curve (4) is apparantly due to a super- 
position of the spectrum of the potassium compound of the nitro- 
samine with that of potassium picrate. From the three bands shown 


1 : 2 
by this curve at A 2000, 2400 and 2900 the latter is undoubtedly 


caused by the presence of potassium picrate, which gives a band at 
about 2880. In the spectrum of the potassium compound of the nitro- 
samine there may be expected two bands at about 2000 and 2350, 
in analogy to the observations made with the other derivatives of 
picrylmethylamide. The former band is indeed present, whilst the 
second band, likely with assistance of the flat band shown by 
potassium picrate at 2500, is transferred to 2400. Two hours after its 
preparation, the alkaline solution of the nitrosamine was again 
examined; it then showed the pure spectrum of potassium picrate 
curve 7). 


The results of this investigation may be expressed as follows. 

The coloration of picrylmethylnitramine by alkali has the same 
cause as the coloration of other derivatives of picrylmethylamide by 
this reagent. 

For the nitramine, the acetyl-, carboxymethyl- and carboxyethyl- 
derivatives, which altogether only have continuous absorption for 
ultraviolet rays, show two bands at about 2000 and 2350 after addition 
of alkali. Picrylphenylmethylamide has already of itself an absorption 
band, which, however, by alkali is divided into two parts at 2070 
and 2400. 


Logarithms of the thickness of the layers in mm. of 0.0002 normal solutions. 


Fig. I. 


651 


16 18-2000) 22) 5524-26) 28-3000) 32, 34 36-38 4000 42 


Reciprocal wavelengths. 


1. 1,3,5-Trinitrobenzene. 2. id. + KOH. 3. Picrylmethylnitrosamine. 4. id. 
+ KOH. 5. Pierylmethylacetamide. 6. id. -+-KOH. 7. Picric acid + KOH, 
8. Methyl picrylmethylaminoformiate. 9. id. -- KOH. 10. Ethyl picryl- 
methylaminoformiate. 11. id. + KOH. 


Logarithms of the thickness of the layers in mm. of 0.0002 normal solutions. 


Vig. 


= 


1 


Bane 


el etl ge ic i 
Pee ere ee ae 
Heyl 

2 AZ 


Bee 


A 
Zoe 
eS 


Za 
eee 


16 


If. 


18 2000 22 24 26 28 3000 32 34 36 38 4000 42 
Reciprocal wavelengths. 


12. Picrylphenyimethylamide (z & @). 13. id. +- KOH. 14. Picrylmethyl- 
amide in sulphuric acid. 15, Pierylmethylamide, 


653 


The nitrogroup attached to the nitrogen atom of the nitramine 
is evidently not essential for the reaction. 

Further, the spectrum of trinitrobenzene with alkali, though much 
differing from that of the other alkaline solutions, has yet its absorption 


1 
in about the same part (> 18002500 ) 


We may thus conclude, that in all these cases the coloration is 
produced by a reaction of the base with one or more nitrogroups 
of the nucleus. 

Finally it bas been shown, that the presence of a strong acid, as 
well as the introduction of acyl radicals, completely expels the absorp- 
tion bands of picrylmethylamide. 


Cheniistry. — ‘“a-Sulpho-propionic acid and its resolution into 
optically active isomerides’. By Prof. A. P. N. Francuimont 
and Dr. H. J. Backrr. 


(Communicated in the meeting of September 26, 1914). 


Already in 1902 a great number of diverse chemical and bioche- 
mical methods were tried by the first of us to separate the e-sul- 
phopropionic acid CH,(SO,H)CHCO,H prepared by him ') from pro- 
pionie anhydride and sulphuric acid, into the two optical isomerides 
that one might expect according to theory. Not a single one, however, 
had given the desired result, although sometimes strychnine 
salts with a different rotating power were obtained, but after their 
conversion into ammonium salts these always appeared to be inactive. 

As Swarts *) had stated that he certainly had obtained from 
fluorochlorobromoacetic acid strychnine salts with varying rotating 
power, but had not succeeded in isolating the optically active acids. 
and as also Poncuer*), who tried to effect a separation of bromo- 
chloromethanesulphonie acid by means of cinchonine, only obtained 
rotating ammonium and barium salts, but no acids, it appeared as 
if with such simple acids the tendency to form racemic mixtures 
or compounds was very great and likewise the velocity of conver- 
sion. This was provisionally also assumed in the case of «-sulpho- 
propionic acid (methylsulphoacetic acid) and the experiments were 
discontinued in consequence. 

Still with lactic acid (methyloxyacetic acid) Purpim and Watknr *) 


MD) TRE, Cl abe, Cla, Gls WAS Zo joo Ad (akststs)\ 
2) Bull. Ac. Belg. (3) 31. p. 25 (1896). 

3) Bull. Soe. ch. (3) 27. p. 438 (1903). 

4) J. ch. Soc. 61. p. 754 (1892). 


and with ebromopropionic acid (methylbromoacetic acid) RaMBERG *) 
had obtained decided results, but on the other hand, Por and Reap *) 
did not sueceed in resolving the chlorosulphoacetie acid. The 
question now arose whether perhaps the sulphogroup created the 
difficulty, i.e. causes the rapid racemisation. This became less 
probable after Pope and Reap *) had succeeded in splitting the 
chloroiodomethanesulphonie acid and had found that the optically 
active acids thus obtained were not so readily transformed into the 
racemie mixture. Hence, the investigation of sulphopropionie acid 
was at once again taken in hand. 

Both ehlorosulphoacetic acid and methylsulphoacetic acid (¢-sulpho- 
propionic acid) are dibasic and thus can form acid salts. Moreover, 
ihe two groups that cause the acid reaction, have a different com- 
position, the one being a carboxyl- and the other a sulphoxyl-group, 
and of different strengtb, so that as the sulphoxyl is stronger acid, 
salts will presumably contain the carboxyl-group in the free and the 
sulphoxyl-group in the combined state. 

Whereas, previously; chiefly the neutral and mixed metallic salts 
and ihe neutral strychnine salt had been experimented with, the 
acid strychnine salt was now employed and the desired result was 
obtained at once. 

a-Sulphopropionic acid itself was hitherto only known as a viscous 
syrup, whilst sulphoacetic acid had been obtained in crystals; 
therefore we have tried also to obtain «-sulphopropionie acid in a 
crystallized condition. 

A dilute solution of the acid prepared by decomposition of the 
barium salt with the theoretical quantity of sulphuric acid was 
concentrated by partial freezing and draining by suction. The strong 
solution was placed in vacuo first over sulphuric acid and then 
over P,O,. The viscous residue was kept for a day in an ice safe 
at about 0°, when gradually large crystals were formed. The acid 
thus obtained contains one mol. of water and is exceedingly hygro- 
scopic. In order to determine its melting point a little apparatus 
was constructed, consisting of two tubes communicating with a 
transverse tube, one of which contained P,O, and the other the 
«-sulphopropionie acid. After the apparatus had been evacuated and 
sealed, it was allowed to stand for a few days. The m.p. of the 
a-sulphopropionie acid was then found to be 100°.5, therefore, higher 
than that of sulphoacetie acid, which is stated to be 84°—86°. 
~ 1) Ber. d. D ch. G. 33. p. 3354 (1900). 

2) J. ch. Soc. 93. p. 795 (1908). 

3) J. ch. Soc, 105. p. 811 (1914). 


655 


An acid strychnine salt was obtained by evaporating an aqueous 
solution of the acid with the equimolecular quantity of strychnine 
on a steam-bath until crystallisation set in. The large erystals that 
had separated were purified by repeated crystallisation from water ; 
their composition then was C,H,O,5 + C,,H,,O,N, + H,O. They, 
however, proved to be not the acid strychnine salt of the inactive 
(racemic) c- ulphopropionie acid, but of the dextrorotatory acid. On 
heating, they are decomposed at about 250° with evolution of gas 
and formation of a brown liquid. 

As in the case of all other compounds described here, the rotating 
power was determined in aqueous solution with sodium light at 20°. 
By concentration c is meant the number of grams of anhydrous 
active substance per 100 ce. solution. The specific rotation [e] is 
likewise calculated on the anhydrous substance. The molecular 
rotation has, of course, the same value for the anhydrous and the 
hydrated crystalline substance. 


For the acid strychnine salt was found at c = 1.938, 
any == — (Sine [41] = — TIA 

By way of comparing, strychnine hydrochloride was also investiga- 
ted and at c=1.297 was found: [a]= —- 30°.2 and | M]—-— 112°’). 


The acid strychnine salt of @-sulphopropionic acid investigated is 
therefore, presumably that of the dextrorotatory acid. 

In order to obtain this acid, the acid strychnine salt was first 
decomposed with the theoretical quantity of barium hydroxide *). 
After complete separation of the strychnine by extracting the drained 
off liquid with chloroform, the neutral barium salt was precipitated 
by addition of alcohol. This salt is dwevorotatory. 

For c=1.764 was found [«]=—4°.96 and [J |= —14°.4. 

From this salt the active a-sulphopropionic acid was liberated by 


3 


1) This value agrees fairly well with the constant |J2]—— 114° found by Porr 
and Reap for a somewhat different concentration. J. Chem. Soc. 105, p. 820 (1914). 

2) The acid strychnine g-sulphopropionate can be titrated with baryta water and 
a suitable indicator such as methyl-red which is sensitive to feeble bases. It may 
also be titrated with litmus to violet-blue. If however, phenolphthalein is used which 
is but little sensitive to weak bases such as strychnine, the colour does not appear 
until also the second acid group combined to the strychnine has been neutralised 
by the inorganic base. As the change in colour is fairly sharp, both with methyl- 
red and phenolphihalein, the titration forms an interesting application of the 
theory of indicators. Still more remarkable becomes the experiment, when 
both indicators are used simultaneously. The methyl-red passes into yellow after 
addition of a semi-molecule of barium hydroxide, the phenolphthalein then being 
still colourless; so soon, however, one mol. bas been added, the violet colour of the 
phenolphithalein salt appears, unaffected by the pale yellow colour of the methyl-red, 


656 


the theoretical quantity of sulphurie acid and its rotatory power 
was then determined. 

For c=0.645 was found [¢]=-+ 31°.6 and [7 ]=- 48°.7. 

In another preparation was found for ¢=1.85, [@]=- 32°.0 
and [J] = + 49°.2. 

Therefore, it is the dextrorotatory acid, whose neutral barium salt 
is laevorotatory. 

It was now tried to obtain also this dextrorotatory acid in the 
solid condition. The solution was, therefore, concentrated in vacuo 
first over sulphuric acid and then over P,O,. The viscous mass did 
not erystallize on cooling, but did so slowly after a trace of the racemic 
compound had been introduced. The crystals are exceedingly 
hygroscopic, melt between 81° and 82° and contain one mol. of water. 

As the neutral barium salt of the dextro a-sulphopropionic acid 
rotates in the opposite direction of the free acid, it became of 
importance to investigate also the acid salt. For this was found 
at c=0.776 

[a] = + 18°.0 and [Af] = -+ 79°.8 or =2 X 39°.9%). 

The acid potassium salt gave at c= 0.516 the valnes: 

[eo] = + 23°.8. [MM] = 4+ 45°.7. 

The acid metallic salts of dextro a-sulphopropionic acid are, there- 
fore, dextrorotatory like the acid itself. The racemisation of dextro 
e-sulphopropionic acid and its salts was also tried. 

The aqueous solution, at c= 0.645, when heated for six hours 
at 100°, suffered no appreciable racemisation, the rotation remaining 
unchanged. 

A solution of the barium salt at ¢ = 1.28 after being heated for 
eight hours at 150° was racemised to the extent of 80°/,. 

A solution of the potassium salt at ¢ = 0.64, which also contained 
2°/, of free potassium hydroxide, was completely racemised after being 
heated for eight hours at 180°. An excess of free base thus seems to 
accelerate the racemisation *), although also the temperature, the 


1) As the molecule of the acid barium salt contains two groups of the sulpho- 
propionic acid, it may for the sake of comparison with the other rotations be 
written more conveniently [IJ] = 2X 39°.9. 

*) This would agree with the rule given by Rorue Ber. d. D. ch. G. 46. p. 845, 
(1914), that active carboxylic acids, the z-carbon atom of which is asymmetric and 
carries a hydrogen atom, are readily racemised under the influence of alkalies. He 
tries to explain this by assuming that, owing to the base, enol formation takes 
place in the molecule, thus causing the asymmetric carbon atom to disappear 
temporarily. 


657 


concentration and the duration of the reaction may exert an 
influence. 

In the motherliquor, from which the acid strychnine salt of the 
dextro-acid had deposited, there should still be present that of the 
laevo-acid, this being more soluble. On addition of acetone a preci- 
pitate was obtained which could be recrystallized from absolute 
alcohol. Of course, it still contains a trifle of the less soluble salt 
of the antipode, but yet in one of the preparations it was obtained 
in a fairly pure condition. 

For the rotating power at c= 1.658 was found [a] = — 27°.7 
and {J/]=-— 135°. The concentration does not seem to exert a 
great influence on the specific rotation, for, at e=8.424 was found 
[a] = — 27°.4 and [M| = — 134°. 

From this acid strychnine salt of the acid the neutral ammonium 
salt was prepared. This gave for c=3.113 the values [a|=-+ 7°.9 
and {J/|—-+ 14°.8. The neutral ammonium salt of the /acid is 
therefore, dextrorotatory. 

If to a solution of the ammonium salt is slowly added dilute 
sulphurie acid, the dextrorotation diminishes, becomes zero and then 
changes to a laevorotation, which finally remains constant, as soon as 
all the erganie acid has been liberated. The rotation for the acid, 
at c= 2.449, amounted to [@] = — 29°.8 and [MM] = — 45°.8. 

Although we have not prepared the /-a-sulphopropionie acid in a pure 
and solid condition, it appears from the experiments in quite a 


d-acid l-acid 
20 20 20 20 
l4Ip | Mp [Ip IM]p 
z-sulphopropionic acid C3H,O;S | + 32? | - 49.2 — 29.8 | =e 
| 
acid potassium salt C;H;0;SK | + 23.8 | + 45.7 | | 
acid barium salt (C3H;0;S),Ba | -- 18.0 | + 79.8 | 
acid strychnine salt leeueoes | 
neutral ammonium salt 
C3H,O;S(NH4), si Oneal 1428 
neutral barium salt C;HjO;SBa| — 4.96 | — 14.4 
| 


658 


satisfactory manner that a resolution has been effected of the racemic 
a-sulphopropionic acid. 

The specific and molecular rotations of the compounds investigated 
are united in the subjoined table. It should, however, be remarked 
that the values of the acid and its derivatives are less trustworthy 
because the acid has not been quite pure. 

It deserves notice that the molecular rotation of the @-sulphopropionic 
acid (49°.2) is certainly somewhat stronger than that of the «-bromo- 
propionie acid *) (44°.4) although the bromine atom (80) differs but little 
in weight from the sulpho-group (81); still this may perhaps support 
the view that the weight of the group influences the rotatory power. 
If for instance, we compare with the rotation of a-ethylpropionic 
acid?) (18°.2) we notice that both the rotation and the weight 
of the group (29) are less. 

More interesting seems the fact that the rotation of the neutral 
metallic salts is much less than, and of an opposite sign to that of the 
acid metallic salts and the acids themselves, particularly in connexion 
with what has been stated at the commencement, namely that it 
concerns here a dibasic acid with two groups of different ionisibility 
which cause the acid functions. 

Although the phenomenon that salts of optically active acids 
possess a rotatory power contrary to that of the acids themselves 
was observed previously, for instance with lactic and glyceric 
acids, the example now found seems a more simple one, because 
there are not present any groups that can react on each other, and 
because it may be called highly improbable that in the circumstances 
stated the carboxyl- and the sulphoxyl-group should react on each 
other. Consequently, the rotation will, probably, be less dependent 
on concentration, temperature, age of solution ete. 

In conclusion, it may be remarked that the laevorotation of the 
acid strychnine salt of the d-e-sulphopropionic acid as compared 
with that of strychnine hydrochloride, amounts to about as much 
Jess as the dextrorotation of the acid metallic salts. 

+) RamBerG. Liebig’s Ann. 370. p. 234 (1909) gives[z] = 29°.0, whence [M] = 44°.4. 


2) Scutirz & Marckwatp. Ber. d. D. ch. G. 29. p. 59 (1896) [z] = 179.85, 
hence [J] = 18.2. 


Physics. - - “A new electrometer, specially arranged for radio-active 
L Oe 
investigations’. Part I. By Miss H. J. Foumpr. (Communicated 


by Prof. H. Haga). 
(Communicated in the meeting of May 30, 1914). 


Introduction. 

In trying to find an accurate method for measurements of the 
natural ionisation of air in closed vessels, radio-active radiation of 
the elements, ete., researches in which very small ionisation currents 
are to be measured, it seemed to me that the need is felt of an 
electrometer, which, besides possessing a great sensibility of charge, 
will also be able to measure very minute currents with accwracy. 

As to the mentioned conditions, the latter is fulfilled by C.T. R. 
Witson’s electroscope (the gold-leaf type), which owes this favour- 
able quality to the very simplicity of the system; this namely renders 
it possible to bring about the ionisation which is to be measured, in 
the air contained in the apparatus itself, to avoid connecting wires, 
together with electrostatic and other influences, the disturbance 
caused by insulators being confined to that of a single one. In my 
opinion this is the reason that this electroscope is generally preferred 
for various measurements requiring great accuracy to say a sensitive 
DoEzALek electrometer, which lacks these advantages, -notwithstand- 
ing the fact of a much greater sensibility of charge of the latter ; 
in consequence of this sudden changes in the natural ionisation of 
air in closed vessels, for instance, the existence of which is accepted 
by many investigators, cannot manifest themselves clearly when the 
electroscope is used; moreover measurements of small currents will 
take much time. 

This has led me to construct an electrometer, the principle and the 
method of working of which I shall discuss in what follows, and 
which in my opinion ean supply the mentioned need. It appeared 
from the results obtained, that with this apparatus currents can be 
measured both very accurately and very sensitively; accordingly 
it seems to me, that for these reasons the apparatus may be very 
suitable for various radioactive researches requiring the above 
mentioned qualities, as was also corroborated by experience. 


Description of the principle of the apparatus. 
In the figure a schematic representation of the arrangement is given’); 
the apparatus consists of: 


1) An accurate description of the apparatus will follow in a 2nd communication, 


660 


two separate spaces, viz. the 
measuring space c: a flat brass 


cylinder, and the ionisation space 
J: a brass cylinder of volume 
1 litre; the two cylinders are 
insulated from each other by 
ebonite. 

In the measuring space is the 
metal needle 6, supported in the 
middle by a second metal needle 
d, insulated by amber; 6 + d 
together form the conductor, which 


is charged by the ionisation current. 

In ¢ is also found the very thin 
aluminium strip a, which a few 
mm. above / is fastened to a thin 
metal rod with mirror, suspended 
on a Wollaston wire, which is 
fastened to a torsion head insulated 
by means of ebonite. 

Through a perforation in the amber and in the ebonite a rod / 
can be brought in contact with the needle d. 

In this way a, 6-+d, ¢, and f, can therefore be separately brought 
in a conductive connection with a storage battery or with earth ; 
e rests on a bottom plate, to which legs are fastened which support 
the apparatus. 


The charging of the apparatus before use. 

In what follows we shall examine from the course of the lines of 
foree, what state arises in the space c, and how this takes place, 
when the system is charged: the lower cylinder f is of no 
account as regards this, as it does not belong to the measuring 
system proper. 

The method of charging is founded on this that the two needles 
a and b, which with untwisted position of a form an angle, let us 
say of 30°, will sé// have this position with respect to each other, 
when the system is in the charged state, in which latter case, however, 
lines of force run between the different conductors. 

We begin to charge a to a constant potential, e.g. to, + 20 
volts, keeping 6 and c still at potential O volt. If for the sake of 
simplicity we first imagine the state as it would be without the 
presence of 6, the course of the lines of foree would be as follows: 
lines of force would start from a, and end upon the bottom, the walls, 


. 


661 


and the lid of c; in consequence, however, of the unequal distance 
from a to those different parts of c, the potential gradient per unit 
of length or the electric force, as also the density of the lines of 
force, or the value of the tensions directed along the lines of 
force in the space round @ would be of very unequal value ; how 
great, however, the variation in different directions might be, yet 
there would be complete symmetry in the course of the lines of 
force with respect to the vertical plane in which the needle itself 
is situated. The presence of /, however, disturbs this symmetry in 
the following way : 

1. The lines of force starting from @ in the direction of ) will 
no longer end on c¢, but on 4; besides, on account of their diminished 
length, therefore on account of the increased electric force, they 
become there denser than before. 

2. There will be inflection of lines of force ; some lines of force, 
viz. those which, when not subjected to the influence of 6, would 
run beside 6 from a to c, will pass into lines of force from a to } 
under the influence of 0. 

This disturbance caused by 6 will give rise to the formation of a 
resulting electrostatic couple, acting on those halves of the side faces 
of a, which are directed to the side of the acute angle between a 
and 6, so that consequently @ is deflected to the side of 6, and the 
angle between a and / will become such that the formed torsion 
couple of the suspension wire will be in equilibrium with the 
electrostatic directive couple. 

In order to make @ return to the untwisted position, ¢ is charged 
to a negative potential, which brings about the desired change; for 

1. then the density of the lines of force between a and ¢ will 
increase, which causes a slighter variation of lines of force on those 
halves of the sides of @ which are directed to the side of the acute 
angle between a and 0 ; 

2. some lines of force between a and ¢/ will deflect and become 
lines of force between a and c. 

In case of a sufficient negative potential of c¢ the above mentioned 
electrostatic resulting couple will be annihilated through this change. 
The course of the lines of force has now become more symmetrical 
(of course not quite), while @ returns to the untwisted position. 

In this way e.g. a state of charge is realized for a= - 20 V., 
H=O V, == 3 

For the sake of simplicity a whole number was taken for the 
potential of c. the consequence of which is, that in the final state 
the needle is only approximately in the untwisted position. 


662 


Measuring method of ionisation currents. 

A quantity of vadio-active substance is placed on the bottom of 
the ionisation cylinder /; the system is charged to the state : + 20 V., 
O V., —3 V.; f is then brought to a potential value, dependent on 
the strength of current to be measured. While a, c, and / maintain 
their potential values, 6 is insulated by breaking the contact with /; 
the ions formed, let us say the positive ones, will then charge 6 to 
a constantly increasing potential, with the consequence that the 
number of lines of foree between a and 4 will decrease, and a 
couple will be formed, which will cause the needles to slowly recede 
from each other, and that the quickeras the current is the stronger 
(to return later on to particulars of the motion). 


Consideration. 

It will be seen from the arrangement of the electrometer, how the 
before mentioned advantages of the Witson-electroscope are. realized in 
it; in the space / namely the ionisation current is directly carried to 
the needle 4+ d, this needle being perfectly insulated by a single 
piece of amber. The separation of ionisation space and measuring 
space has, moreover, this advantage that the measuring system is 
not contaminated with radio-active impurities, while the ionisation 
space and the rod d, which can be removed, as regards the part 
that lies in 7, can be easily cleaned. 

As to the measuring system proper, the principle of it differs from 
that of the quadrant electrometer; it has been thus chosen on purpose 
that the lines of foree formed by the ionisation current contribute 
as much as possible and as favourably as possible to the movement 
of the needle a. 

This is not the case in the quadrant electrometer; there namely 
the movement is caused by the lines of force which run between 
the quadrants and the rims of the needle, whereas the vertical lines 
of force between needle and quadrants do not contribute anything to 
the moving couple. 

In my opinion it would not be possible to modify the quadrant 
electrometer in such a way that, while maintaining the principle of 
the quadrants, many lines of force are not retained at the same time 
which in a measurement either give no movement, or will even 
counteract the movement. The latter might be possible, if the flat 
needle should be replaced by a horizontal wire, in which way a 
large horizontal surface is, indeed, avoided, but on the other hand 
the formed lines of force would act on the two sides of the needle, 
when the latter is rotated. The advantage of the described apparatus 


663 

lies in this that the lines of foree between a and 6, which ave 
subjected to a change on ionisation, will mostly arise on one side 
of the vertical strip. This removes the last mentioned drawback, a 
large injurious horizontal surface also being avoided. I think that 
with this apparatus I have obtained a sensibility of charge, greater 
than is possible with a DorezainK-electrometer, the same thickness 
of wire given. 


The realization of a greater sensibility of charge. 

-The sensibility of the apparatus appeared to be capable of great 
variation, the suspension wire being left unaltered, and that by 
varying the state of charge, whereas, for the rest, the method of 
charging and measuring remains the same. To make the system 
more sensitive, a is not charged to + 20 V, but say to +32 V, 
after which a negative potential value is imparted to ¢ such that a 
has turned back to an almost untwisted position. The potential of 
e will also be more strongly negative, of course, for this state than 
for the state (+ 20.0, 
e.g. (+ 32,0, —6) V. 

In order to understand what causes this modification of charge to 
bring about greater sensibility of charge, we must examine in the 
apparatus 1. the variation of the potential sensibility. 2. the variation 
of the value of the capacity; for these two factors together determine 
the sensibility of charge. 

1. The former is to be found from the curves I, in which examples 
of some states of charge are given; to investigate the potential 


3) V; the state of charge will then become 


z 
S 
& 50 
— 
Ss 
o 
S 
o 
= 
a 25 
2. 
fe 
Q 
0 
ry) 30 Votts 20 
Fig. 1. 
44 


Proceedings Royal Acad. Amsterdam, Vol. XVII. 


664 


sensibility & was increased every time by 2 Volts in potential 
for every state separately. The state, as indicated over every 
curve, always represents the initial state. All the measurements 
following here were made with a provisional apparatus; the suspen- 
sion consisted of a Wortaston wire 7m thick, and 97 mm. long. 
(Seale distance 1.5 m.). 

From these curves appears the greater potential sensibility of 
the system for greater potential difference between a and 6; for the 
state (+ 32.0, —6) V e.g. a displacement of almost 700 mm. was 
fuund for 2 V potential increase of 4; for (+8.0, —2) V it amounted 
to +500 mm. for 20 Volts. The state (+382.0,—6) V does not 
represent the most sensitive state that could be obtained. 

I think the cause of this greater potential sensibility is the 
following : 

When a recedes from / in consequence of a potential increase 
of 4, which is brought about by increase of charge of 6, the negative 
induced charge on 6 will diminish in consequence of this motion, 
or rather the potential value of 6 will be diminished ; for a positively 
charged body (a) recedes from 6. The greater the potential difference 
is between a and #, the greater will be the potential diminution in 
question for a definite angle; in other words the potential diminution 
of 6 required for a receding of a over a definite angle will be the 
less, i. e. the potential sensibility will be the greater. Besides the 
said change of the induced charge at the same time increases the 
angular displacement, which is another reason for greater potential 
sensibility. 

2. It follows from the foregoing, that greater potential sensibility 
obtained in this way, must be attended by an increasing capacity ; 
for when through a definite addition of charge to 4 in a state with 
greater potential difference between a and + a slighter potential 
increase will set in in consequence of the motion of a, this will imply 
a greater capacity of 4. Capacity measurements (method Harms, 
Phys. Zs. 1904) give the same result; the capacity in the state 
(+ 8,0—2) V amounted namely to 5,2 e.s. units; that in the state 
(+ 20,0—3) V 6,0 es. units. Both values are the mean from a great 
many determinations. 

What is the reason why, in spite of this increase of capacity, the 
increase of potential sensibility more than counterbalances it, will 
appear from the application of the following consideration of the 
capacity. 

Though for an electrometer the sensibility of charge is in direct 
ratio to the potential sensibility, and at the same time in inverse ratio 


665 


to the value of the capacity, it does by no means follow from this 
that the sensibility of charge will be greatest for a capacity as small as 
possible, and a potential sensibility as great as possible; for the latter 
quantities are not independent of each other, as appears clearly among 
others in what was said under 2. therefore I cannot entirely concur 
with Lasorpk’s statement, in his: ‘‘Methodes de mesure, employées 
en radioactivité, page 66”, where he says: “l'appareil le plus sensible 
aura une grande sensibilité aux Volts et une faible capacité”; in 
this statement the above mentioned relation is namely not taken 
into account. 

Thus in consequence of the existing mutual dependence of capacity 


and potential sensibility it will be possible — and it will be shown 
here that this really applies to the discussed electrometer —_ that 


it will be favourable for the sensibility of charge, to take the capacity 
not as slight as possible, when namely an accompanying increasing 
potential sensibility more than compensates the disadvantage of 
this procedure. 

That this case presents itself in the described apparatus may be 
shown by first examiming of what the capacity of the apparatus, i.e. 
of the needle 6-++-d really consists. This capacity consists of : capacity 
of the part 6, which refers to arising or vanishing lines of force 
leading to a or c, and capacity of d. 

Now | would distinguish in this capacity between: 

a. useful capacity, by which I mean capacity which has an influence 
on the motion of a; 

b. injurious capacity which lacks this influence, and which is really 
a disadvantage here, because it binds charge of the ionisation 
current without making it demonstrable. Of the above mentioned 
capacity only that corresponding to the lines of foree between a and d 
is certainly almost entirely useful capacity (see below); the rest is 
injurious. 

And in this lies the cause why the state with greater potential 
difference between a and 6, though attended with greater capacity, 
can yet mean greater sensibility of charge; for this increase of capacity 
concerns here the capacity of 4 with respect to a; this is increased, 
(according to 2) hence the useful capacity of 6 is increased; the 
greater now the ratio of useful to injurious capacity is, the greater 
the sensibility of charge. 

For the rest, as regards the value of the injurious capacity in the 
apparatus, the following remarks may be made: 

1. The injurious capacity of d with respect to / will not be of 
great influence, since the distance to / is great. 

44% 


666 


2. So far the lines of force starting from the lower rim of a, or 
from the back of a, ending on 6, were not taken into account; 
they represent injurious capacity. This influence will make itself 
slightly felt in the middle of the needle, but will nave little effect 
there on the motion. 

3. It is difficult to say anything definite about the value of the 
injurious capacity of b with respect to ce. 

At any rate it will also appear from what follows, how for very 
sensitive states the total influence of the injurious capacity may 
almost be disregarded. 

In the case of the quadrant-electrometer, on the other hand, the 
injurious capacity is that of large surfaces with respect to a metal 
needle lying close by. 

Before confirming what has been said above about this increased 
sensibility of charge for greater potential differences between a and 
b by the communication of some experimental results, a few par- 
ticulars may be added abont the mode of motion of the needle 
during the current measurement. 

Mode of motion of the needle during the current measurement : 

When the needle 4 is charged starting from potential 0 V_ by 
means of an ionisation current, when therefore the potential 
difference between a and / decreases, a will begin to move away 
from 4; consequently a motion of the scale division under the 
crosswire will take place through the reflection of the mirror, which, 
however, will not be uniform. For the different positions occupied 
by a both the potential sensibility and the value of the capacity of 
6 will be different; for the smaller the angle with b, the greater is 
the potential sensibility, as well as the capacity. 

The causes are the following: 1. With a smaller angle the distance 
between qa and / is smaller and therefore the diminution of the 
induced charge for a definite change of angle greater. 

2) With a smaller angle the potential difference itself is also 
greater, and this again causes a greater decrease of induced charge 
for a definite angle. 

For both reasons greater potential sensibility, but at the same 
time greater capacity is to be expected at a smaller angle, but here 
too for the same reason as for conditions of charge with greater 
potential difference between a and 6, the result will be a greater 
sensibility of charge 

In agreement with this the curves I show, how for every state of 
charge the potential sensibility decreases with greater angle between 
a and b, 


Capacity determinations gave the further result that the capacity 
amounted to 5.75 e.s. units for the state (+ 20,0—3) measured from 
an angular displacement (recession), corresponding to 550 mm. seale 
displacement, whereas it gave the value 6 e. s. units, when this dis- 
placement only extended over 250 mm. 

Measurement of the current. 

With the different above mentioned states of charge ionisation 
currents were measured, obtained with two different very slight 
quantities of polonium, which were placed in a dish on the bottom 
of f; the larger quantity is called A, the smaller 4. The velocity 
with which the scale moved under the cress wire was determined, 
and then the intensities of current were derived in absolute measure 
from this by means of the knowledge of the capacities and potential 
sensibilities holding for some of the states of charge. 

The curves IL. represent the result of the measurements for the 
quantity A; it appears from this, that in accordance with expecta- 
tion the sensibility of charge increases for states with greater potential 
difference between a and (; at the same time this confirms what 


60 p a 


40 


Sensibility of charge 


Displacement in cm. 
ts) 


o aco seconds 400 
Fig. 2. 


was discussed before, that namely the sensibility of charge for one 
and the same state is greatest, when @ is nearest 0. 

From the experiment in itself the ratio of the current intensities 
of the two quantities of polonium could already be derived, and 
that even for each state of charge taken by itself. It will namely be 
equal to the ratio of the times required by a to pass through the 
same angle for the quantity 4 and for B. This ratio, which would 
have to yield the same value for every state of charge, amounted 
successively to 2.5, 2.7, 2.7, mean 2.6. 

According to the above it was now possible at the same time 
by means of the measured capacities and the known potential sen- 


668 


sibilities to determine the currents for A and B in amperes, from 
CX V-inerease per sec. . : 
the formula : 44 == = in which C represents 
SS) S< AKOee 

the capacity of the needle / +d. As mean values from the values 
for the 3 most insensitive states we thus obtained : 

14 = 1.3 X 10-8 (quantity B) 

24 Ore >< 10718 ( 5p A) 

Limits of sensitiwity of the apparatus. 

Besides being dependent on the state of charge of the system, the 
sensibility of charge can also be modified by varying the thickness 
of the suspension wire and the angle between the needles. 

It was now of interest to ascertain how far the influence of 
a change of the state of charge in this respect could extend, how 
far in other words the apparatus might gain, resp. lose sensibility 
of charge by a constantly increasing or diminishing potential difference 
between a@ and 6. Experiment showed, that there are limits on either 
side, at which the apparatus presents a very peculiar character ; 
this will successively be examined for a smallest sensibility, and 
then for a greatest sensibility. 


a, Limit of smallest sensibility. 

Though for the just mentioned state of charge (-+ 8, 0, + 2) V 
the phenomena were similar to those for the other states of charge, yet 
the limit of sensibility appeared to be close in the neighbourhood, 
viz. at the state: (+ 4,0,0) V; this will most clearly appear from 
the experiment in which the potential sensibility was examined by 


| [ te aie 
0 5 7 =T = 
\ | IL Behaviour of the most insensitive state 
Sg 
° 6 =e = = 
= 
5 7 
g XN 
ee nN 
a 5 ic at S = al 
SNe 
21 eae 
0 36 Volls 32 


669 


the regular increase of the potential value of 4. It appears from 
curve III how, in contradistinection with the other states, @ first 
recedes from 6, and then approaches 6 again. 

The explanation of this deviation from the ordinary phenomena 
is very obvious; for the potential value of a being low, 6 will soon 
rise above this value in potential value, and this more and more; 
hence the diminution in lines of force between a and 6 first con- 
tinues, till the potential value of 6 has risen to +-4V; then lines 
of force arise again between a and 6, whose number increases with 
the rise of the potential of 4, so that finally the needles will, instead 
of receding, approach each other. 

In accordance with expectation it appeared from the experiment 
for the current measurement that the needle first receded from 4, 
stopped, and then approached 0. 

This state of charge appeared, therefore, to be unsuitable for the 
current measurement, of course under for the rest entirely definite 
circumstances of thickness of wire, height, and angle of the needles. 

b. Limit of greatest sensibility. 

In the following examples of states of charge illustrating this 
case a certain difference with the foregoing ones may be observed; 
for the rest this modification was taken voluntarily; 6 is here 
namely in the initial state already at positive potential, while the 
potential value was /owered during the measurement, in other words 
in contrast with the preceding cases a approached to 4 through 
increase of the lines of force between a and 6. 

In the following examples the potential decrease for 4 amounts 
every time to 2V, and it is always stated how much then the 
deviation is for a, expressed in mm. of scale displacement. 


A) state (+ 80, +60, +60,) V.| (2) state (+80, +40, + 36,) V. 


GED Se Vi S2smm: b +838 V. 130 mm. 
ss q 513 , 6) 55 + 36 af Oe 
apo“ 71) 4 | » +24 ,, theneedle 


A SEPIA aE ae | turns. 
ie state) (meet) ees 
(3) state (+80, + 30,+26,) V.| (4) state (+ 80, +10, +4,) V. 
iy arts) Wo Oils | b +8 V.  theneedle 
>» 26 5, theneedle | turns. 


turns. 
(5) state (+ 120, + 40,+ 32) V.| (6) state (+ 120, +10, +2) V. 
6 + 388 V. the needle 6 + 8 V. the needle 


turns. | turns, 


The phenomenon that occurred now was the following: when e.g. 
in the 3 state 6 was charged to + 26 V, after having first been 
brought to -+- 28 V, we did not once more observe a deviation which 
amounted. to somewhat more than that for the change of the 
potential value of 6 from -+ 30 V to + 28 V (since the sensibility 
at smaller angle zncreases), but a passed over so great an angle that 
the whole scale disappeared from the field, and a assumed almost a 
position parallel to 6: the needle turned suddenly. In state 4 this 
phenomenon occurred immediately at the first potential decrease of 
b with 2 V, and the sume applies to the 5 and 6" states, 
whereas in contradistinetion with this the first state exhibited stable 
states throughout the scale for definite potential values of 0. 
The experiment seemed therefore to point to the existence of an . 
unstable state of equilibrium of a, which gradually shifted to an 
increasing angle with 6 as the state of charge became more sensitive. 
To ascertain, whether this displacement was a gradual one, the 
inrning point was approximated as nearly as possible for every state 
separately; this was done by diminishing ® in potential value not 
by 2 Volts every time, but only by parts of 1 Volt. The result of 
this was that, as had been expected, the 2"¢ and 38'¢ states were 
still realisable throughout the scale, the 4", 5, 6 states on the 
other hand only partially, but again in such a way that the said unstable 
state of equilibrium, hence the turning point, occurred at a greater 
angle, as the state of charge was more sensitive. 

When after the turning a had reached its new state of equilibrium, 
it was not possible to make a return to its position through a slight 
potential increase of 4, which, considered in itself, would give rise 
to a state of charge with a stable equilibrium ozéside the region of 
turning. This too pointed to the existence of an unstable equilibrium. 

The explanation of the existence of such an unstable equilibrium 
at the point of turning seems to me the following : 

In what precedes the change was already discussed of the 
induced charge on 6, in consequence of an angular displacement 
of a; we saw how this change takes place for a definite angular 
displacement to a greater degree, the greater the potential difference 
is between a and 4, and the smaller the angle is between the needles. 

Taking this into consideration we may ask what will take place 
when e.g. the state (+ 83, + 30, + 26,)V is realized, and when 
the negative charge is continually supplied to 6. 

In this the ratio of useful to injurious capacity will namely con- 
tinually change for the before-mentioned reasons; it will become 
continually greater; at a definite angle the influence of this injurious 


capacity can even ‘all but vanish. This circumstance can also be 
expressed thus, that then even a supply of negative charge will no 
longer make the potential of 4 go down, because the approach of 
a to 6 brought about by this supply just compensates the expected 
potential decrease. 

The angle, for whic) this consideration holds, will still be found 
outside the region of turning and may be realized by means of a 
storage battery. 

If more and more negative charge is added at this angle to 4, e.g. 
through an ionisation current, the potential value of 6 will even 
continually rise in consequence of the preponderating influence of the 
approach of a to 6. Finally the state becomes this, and it is then 
that the turning takes place, that for a further approach of a toda 
supply of charge to / is not even required any longer. For the mere 
induced charge on 6 called forth by the approach will be more 
than sufficient to give rise to an electrostatic couple, which can be 
in equilibrium with the formed torsion couple. 

That, however, in case of such a turning the parallel state is not 
entirely reached, which was already pointed out, may be accounted 
for in this way that the lines of force between a and 6 at decreas- 
ing angle will also act on the back of a in appreciable quantity, 
and this more and more as the angle becomes smaller, so that through 
this circumstance the electrostatic couple, which tends to make the 
angle between a and 6 smaller, is counteracted. It will follow from 
this, that after the turning, the two needles will always continue to 
form a (generally small) angle with each other. 

It follows therefore from this explanation of the angle of turning, 
as was already pointed out on p. 47, that, when the measure- 
ment is made in the neighbourhood of this angle, the capacity which 
must then be taken into account, will chiefly consist of useful capacity, 
by which the sensitivity of the state is to be explained. 

In conclusion a single example of a measurement of air-ionisation 
and of Rubidium-ionisation. 

In thcse measurements the needle a@ was brought to potential zero ; 
the state of charge was: 0 V., — 26 V., — 32 V. 

The ionisation space contained only air; volume 1 litre; the 
number of seconds successively found for the passage through 10 mm. 
WAS Low dewolemont Ooq Hae 

Then a quantity of Rubidium salt was placed in a dish with an 
area of.50 em’, on the bottom of /; it was found that successively : 
9, 10, 10, 11 seconds were required for the passage of 20 mm. In 
this case 7 was at + 80 V. 

Physical Laboratory of the University at Groningen. 


672 


Chemistry. — “The metastable continuation of the mixed crystal 
series of pseudo-components in connection with the phenomenon 
allotropy”. Il. By Prof. A. Smits. (Communicated by Prof. 
J. D. vAN DER Waals). 


(Communicated in the meeting of Sept. 26, 1914). 


In the first communication on this subject ') different possible 
continuations of the mixed crystal series in the metastable region 
have been discussed, in which chiefly the mixed crystal phases 
coexisting with liquid were considered. 

The metastable continuation of the coexistence of two mixed crystal 
phases was only mentioned in a single case, where namely continuity 
of the mixed erystal phases in the metastable region was supposed. 

It is now, however, the question what can be said of this 
coexistence for the case that the said continuity does not exist. We 
consider, therefore, one of the figures from 7 to 12 inclusive from 
the previous communication, and ask what can be predicted about 
the metastable continuation of the lines p and m. 

On the whole a transgression of the melting temperature without 
melting setting in, or in otber words supersolidification, is considered 
possible also on slow rise of temperature. The continuity discussed 
by Vax per Waats between the sublimation line a 6 and the melting 
point line 4c of a single sub- 
stance, see fig. 1, starts from 
this supposition; we shall, there- 
fore, also here have to take the 
possibility into account that the 
melting fails to appear at the 
eutectic temperature, and_ that 
the coexistence continues to exist 
between the two mixed crystal 
phases. It is, however, the ques- 
tion whether this possibility is 
limited. It follows from the con- 
tinuity between the sublimation 
line and the melting-point line 
considered by vAN DER WAALS that 
such a limit has been assumed 
for the coexistence between solid + vapour and solid + liquid. 


1) These Proc. XVI p. 1167, 


673 


Above the temperature of the higher cusp e, and below the pressure 
of the lower cusp d, the solid substance can no longer exist by 
the side of the gas resp. liquid. 

For our purpose the cusp c is the most important, for this point 
expresses that there exists a limit for the coexistence solid + gas, 
which implies that the orientated condition of the molecules in the 
solid substance coexisting with its vapour cannot exist any longer 
at a definite temperature, in consequence of the increasing molecular 
motion. If this holds for the solid substance in coexistence with 
vapour, there must also be a limit of existence for the solid substance 
without vapour, and as the contact with the vapour will diminish 
the stability of the solid state in consequence of the molecular 
attraction between the molecules in the solid phase and those in the 
gas phase, we may expect that the limit of existence of the solid 
substance without vapour will lie at a higher temperature. This 
temperature limit of existence will vary with the pressure, and thus 
we shall be able to draw a line wv in the P7-figure indicating the 
limit of existence of the solid substance. 

For a binary system this holds of course, for both the components. 
When, therefore, we pass from the triple point of the components 
to the quadruple point, we get something similar. As Dr. Scurrrmr 
has demonstrated ’) and as is expressed in Fig. 2, the lines for 
Sat Se+ G, Sit Spg+ L merge continuously into each other 


also by means of a ridge with two cusps and an unstable inter- 


1) These Proc, XIII p. 158, 


674 


mediate portion, and here a line pg can be given for the limit of 
coexistence of S4+ Sg, because either S4 or Sp has reached its 
limit of coexistence there, which makes it impossible for the said 
coexistence to occur any longer. 

It follows therefore from this that the lines p and m extend 
metastable to a definite temperature above the eutectic one. 


Transition from monolropy ¢o enantiotropy. 


As is known it often happens that a substance under the vapour 
pressure presents the phenomenon of monotropy, whereas under 
higher pressure enantiotropy takes place, as has e.g. been indicated 
in the P7Z-figure 3. 

The theory of allotropy again enables us to get a clear insight 


into the signification of this phenomenon. 
Suppose the 7. X-figure 4 to hold for a pressure above the triple 


point O, and below the triple point O,, then according to the said 
theory the conclusion may be drawn from the fact that at higher 
temperature enantiotropy occurs, that the situation of the internal 
equilibrium with respect to the pseudo system is dependent on the 


pressure. For only in this case e.g. the situation of the line for the 
internal equilibrium in the liquid with respect to the pseudo system 
will shift with the pressure, and if this displacement is such that 
the point /, moves downward with respect to the pseudo binary 
T,X-figure, /, will coincide with c, S, with d and S, with e at a 
given pressure, or in other words under this pressure two solid 
modifications of the unary system will be in equilibrium with each 
other and with their melt at a definite temperature (triple point 
temperature). 

At this temperature the two modifications have therefore the same 
melting-point pressure, so that this temperature can also be ealled 
a transition temperature under the melting-point pressure. 

If we raise the pressure still more, we get a 7\r-figure as given 
in Fig. 5, from which it appears that whereas the direction of the 
lines for the internal equilibrium in the solid phase excluded: the 
appearance of a stable point of transition at lower pressure, it must 

now at higher pressure neces- 
¢ sarily lead to a transition point. 

We see further that the solid 

phase which appears at the 

stable point of solidification now 
lies on that mixed erystal line 
on which the solid phase of the 
metastable melting equilibrium 
lay before, and vice versa, so 
that the form of erystallisation 
of the solid phase at the stable 
point of solidification will now 
be equal to that in which the 
metastable phase showed itself 
at a pressure be/ow the transi-’ 
tion pressure. 

On further increase of pressure 


EE ea & the puints /, and s, move still 


Fig. 5. more to the left, and the transi- 
tion equilibrium gets deeper and deeper below the equilibrium of 
melting. 

The P, 7-projections of the points s, and /,, at different pressures 
will form the stable melting-point line, that of the point s, and /, 
the metastable one, whereas those of the points s’,, s', form the 
transition line as indicated in fig. 3. 

It therefore appears from the foregoing that the transition from 


676 


monotropy into enantiotropy can be explained in a simple way 
by means of the theory of allotropy. 

Now the question rises where the transition line eo, starts from. 
A possibility has been given in fig. 3, from which follows that the 
transition line starts in a metastable point of transition under the 
vapour pressure O,. This is the view to which lead Ostwatp’s *) and 
Scuaum’s*) assumptions on the existence of a metastable point of 
transition under vapour pressure*). Now it is the question whether 
this is the only possibility. It has been pointed out just now that 
the metastable coexistence is confined between the two mixed erystal 
series md and pe (see Fig. 4), and as the metastable point of 
transition arises by intersection of the internal equilibrium line of 
the solid phases with the above mentioned mixed crystal lines, it is 
clear that it may happen that this intersection does e.g. noé exist 
under the vapour pressure. 

If in such a ease enantiotropy does oecur at higher pressure, the 
transition line will proceed in a metastable way up to that pressure 
and that temperature at which for the first time an intersection 
between binary mixed crystal lines and internal equilibrium lines 
takes place, and there the transition line will then suddenly terminate 
in a point that indicates the 
limit of existence of the 
coexistence between two solid 
phases which are in internal 
equilibrium, as fig. 6 shows. 

Now it is clear that the 
main cause of the transition 
from monotropy to enantio- 
tropy can jind its origin 
exclusively in this that the 
situation of the pseudo figure 
varies more greatly with the 
pressure than that of the 
unary figure, but in by far 
the most cases, namely there 
where the pseudo components 

Fig. 6. are different in molecular 
sizes, the situation of the pseudo figure will vary less with the 


1) Z. f. phys. Chem. 22, 313 (1897). 
2) Lieb. Ann. 300, 215. 


*) Cf also Bakuuis Roozesoom, “Die Heterogenen Gleichgewichte” I, 187. 


677 


pressure than that of the internal equilibrium, and the phenomenon 
discussed here will have to be attributed to this superposition. 

In conclusion it may be pointed out that other particularities may 
still present themselves, when the internal equilibrium line of the 
liquid phase under the vapour pressure lies so much on one side 
that there exists no meta- 
stable melting point under 
this pressure. If we now 
think that this case occurs, 
and that the internal equili- 
brium line for the liquid 
phase under the vapour 
pressure lies greatly on 
one side towards the right, 
and that this line moves 
towards the left on increase 


of pressure, we get what 
follows: The phenomenon Fig. 7. 

of phase allotropy’) is wanting under the vapour pressure, monotropy 
can however, occur at higher pressure. 

The metastable melting-point line will start at the absolute zero 
e.g. in the case of fig. 10 of the preceding communication *), and 
run further as represented in fig. 7. 

If on the other hand we have to do with the ease of fig. 12 of 


Fig. 8. 


1) For the occurrence of a substance in two or more similar phases the word 
phase allotropy might be used, while the occurrence of a substance in different 
kinds of molecules, for which I before introduced the name homogeneous allotropy, 
might be designated by molecular allotropy. 

2) loc. cit. 


ihe preceding communication, a P7-figure is possible as fig. 8 shows. 

These considerations open our eyes to the possibility that enantiotropy 
occurs under higher pressure, notwithstanding the phenomenon of 
monotropy is not found wader the vapour pressure, 


Amsterdam, June 25, 1914. Anorg. Chem. Laboratory 


of the University. 


Chemistry. — “On the vapour pressure lines of the system 
phosphorus.” (Ul. By Prof. A. Smits and 8. C. Boksorst. 


(Communicated by Prof. J. D. van per Waats). 
(Communicated in the meeting of Sept. 26, 1914). 


The continued investigation of the phosphorus purposed to decide 
with certainty whether the red and the violet phosphorus must be 
regarded as two different modifications exhibiting the phenomenon 
of enantiotropy, as seemed to follow from Jonipors’') researches and 
also from our first investigations. 

Confining ourselves te the communication of the result we can 
state with certainty that the supposed point of transition between 
red and violet phosphorus does uot exist, and that only one solid 
stable modification of the phosphorus has been found, which is violet 
in coarser crystalline state, but red in a more finely divided state. 

The vapour tensions of different phosphorus preparations approach 
to amounts which form one continuous vapour pressure line, when 
the heating is long continued. 

An apparent discontinuity may arise under definite circumstances 
in consequence of too rapid heating. If namely, the preparation at 
lower temperature contains too much of the more volatile pseudo- 
component, too high vapour pressures are observed at these lower 
temperatures, in consequence of the not setting in of the internal 
equilibrium. In the neighbourhood of 450°, however, the setting in 
of the internal equilibrium becomes appreciable, and this transformation 
being attended with a diminution of the vapour pressure, the vapour 
pressure line will present a course that reminds of a discontinuity. 
When we worked very slowly and started from states which could 
only differ little from internal equilibrium states, any discontinuity 
had, however, disappeared. 

At the same time this investigation furnished a fine confirmation 


1) CG. R. 149, 287 (1909) and 151, 382 (1910). 


679 


20 


10 


he 


300° 350° 400° 450° 500° 550° 600° 


Vapour pressure line red phosphorus determined by means 


of the glass spring indicator, 


— = —_ — SS 
| Vapour pres- ; Vapour pres- | 
Temperature | Sarena atin | Temperature "sure in atm. 
(e) (eo) | 
300 0.05 480 5.0 | 
325 0.1 490 6.25 | 
350 0.2 500 esl | 
375 0.4 510 9.4 
400 0.7 520 2 
410 0.9 530 PiS32 
420 15 540 15.65 
430 1.55 550 18.75 
440 1.90 560 22.95 
450 2.45 570 28.6 | 
460 3.15 580 35.6 
470 4.0 589.5 43.1 Triple point 
45 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


680 


of the theory of allotropy, as it necessarily led to the conclusion 
that the stable red or violet modification is really complex, and 
consists at least of two components, which greatly differ in volatility. 

As the denomination ved phosphorus is universally known, we 
will also apply this term to the stable modification, though, as was 
said before, this modification is violet in coarser crystalline state. 

The adjoined figure represents the vapour pressure line, as it has 
been found by us after laborious study, and the table gives the 
vapour pressures at different temperatures, as they can be read from the 
vapour pressure line. In a following communication this investigation 
will be treated more fully. 


Amsterdam, Sept. 25, 1914. Anorg. Chem. Laboratory 
of the University. 


Chemistry. — “The application of the theory of allotropy to electro- 
motive equilibria.” IL. By Prof. A. Smits and Dr. A. H. W. 
Atrrn. (Communicated by Prof. J. D. van DER WaAats). 


(Communicated in the meeting of Sept. 26, 1914). 
Introduction. 


The application of the theory of allotropy to metals necessarily 
led to the assumption that every metal that exhibits the phenomenon 
of phase allotropy, must contain different kinds of ions. As was 
already mentioned before, these kinds of ions can 1. differ in com- 
position, the electric charge per atom being the same; 2. differ in 
valence with the same composition, and 3. differ in composition and 
charge per atom. 

On extension of the said theory to the electromotive equilibria it 
was now demonstrated 1. that the unary electromotive equilibrium 
finds its place in a Aw figure of a pseudo system, 2. what can be the 
relation between the unary and the pseudo-binary system, and 3. what 
phenomena will have to appear when in case of electrolytic solution 
resp. separation of metals the internal equilibrium is noticeably 
disturbed. The phenomena of anodic and cathodic polarisation appeared 
by this in a new light and the passivity of metals revealed itself as 
a disturbance of the internal equilibrium in the metal surface in the 
direction of the noblest kind of ions’), which view seemed already 
to be confirmed by a preliminary investigation *). 

Thus we had arrived at the region of the passivity of metals, and 
!) These Proc. XVI p. 699. 

*) These Proc. XVII p. 37. 


681 


it became desirable to get acquainted with the immensely extensive 
literature on this phenomenon. 

The most important hypotheses that have been proposed as an 
explanation of this phenomenon, and which have been collected by 
FREDENHAGEN ') in an interesting summary, are the following: 

1. The oxide theory of Farapay, who assumes that passive metals 
are covered by a coat of oxide *). 

2. KriGer FINKELSTEIN’s *) valence theory which slightly modified is 
also adopted by Métrer‘). In this it is assumed that the passivity 
consists in a change of the proportion between the components of 
different valence. 

3. Le Buianc’s velocity theory *), which supposes the phenomena 
of passivity to be due to the slight velocity with which the formation 
of metal ions would take place. 

4. The velocity theory of FREDENHAGEN °), MutHmMann, and FRAUvEN- 
BERGER’), who start from the supposition that the passivity is caused 
by the slight reaction velocity between the anodically separated 
oxygen and the passifiable metal, which causes oxygen charges or 
solutions of oxygen in metal to originate. 

5. The theory of Grave‘), who assumes a retarded heterogeneous 
equilibrium metal-electrolyte which is under catalytic influences. 

If we now consider the passivity which has arisen by an electrolytic 
way, it seems to us that too little attention has been paid to the 
primary character of the phenomenon. 

First of all we should inquire to what it is owing that in case of 
anodic polarisation of base metals the potential difference is modified 
in such a way that the tension of separation for the O, is reached, 
and we should also question why in case of cathodic polarisation 
of base metals the potential difference changes in such a way that 
the tension of separation for the H, is reached. 


1) Z. f. phys. Chem. 63, 1 (1908). 

®) Farapay has not expressed himself so positively as is generally thought. In 
a letter to R. Taytor Farapay writes explicitly [Phil Mag X 175. Jan. 2! (1837)]: 
“IT have said (Phil. Mag. IX. 61 1837) that my impression is, that the surface of 
the metal is oxidized, or else, that the superficial particles of the metal are in 
such a relation to the oxygen of the electrolyte as to be equivalent to an oxidation, 
meaning by that not an actual oxidation but a relation... 

8) Z. f. phys. Chem. 39, 104, (1902). 

) Renee re » 48, 577, (1904). Z. f. Electr. Chem. 11, 755, 8238, (1905) 

5) Chem. News 109, 63 (1914). 

6) Z. f. phys. chem. 48, 1 (1903). 

7) Sitzber. K. Bayr. Akad. 34, 201 (1904). 

8) Z f. phys. Chem. 77, 513 (1911). 

45* 


682 


These phenomena being only observed above a certain current 
density, it is clear that we have to do here with a disturbance 
which makes its appearance when the electric current is passed 
through with too great velocity. 

We have, therefore, to do here with a question of velocity, and 
as an explanation of the primary character of the passivity pheno- 
menon Farapay’s oxide theory is to be rejected from the beginning. 

With regard to Grave's theory we may remark that it seemed 
very improbable already at a cursory examination, Nernst has 
namely demonstrated that in the phenomenon of solution equilibrium 
of saturation always prevails in the boundary layer solid-liquid. In 
connection with this we may, therefore, expect that this continues 
to hold for the phenomenon of solution by an electrolytic way. 
There is no reason at all to make an exception here. 

With regard to the second theory it should be observed that the 
valence hypothesis, on which it is founded, is implied in the con- 
clusions to which the application to metals of the theory of allotropy 
leads. This theory generally concludes, namely, as was already said 
before, to the existence of different kinds of ions in the metal phases 
and points out that one of the possibilities is this that the metal ions 
with the same composition only differ in valence. 

The application of the theory of allotropy to the heterogeneous 
electrolytic equilibria has further shown that when the metal phase 
is complex, apart from the nature of the difference between the ions, 
the anodie and cathodie polarisation, and also the passivity of metals 
can be explained. 

Diametrically opposed to this theory are the theories 3, 4 and 5, and 
it is now clear what will have to be decided. By an experimental 
way we must try to get an answer to the question as to whether 
the phenomenon polarisation and’ passivity resides in the boundary 
surface between metal and electrolyte, as the theories 3, 4 and 5 
suppose, or in the metal surface itself, as the theory of allotropy 
has rendered probable. 

For this purpose the investigation about the complexity is the 
obvious way. When experiment has proved the complexity, we can 
try to find out whether it possesses metal ions of different valence. 


Experimental part. 


1. To examine whether or no the phenomenon of polarisation and 
that of passivity resides in the metal surface, it seemed to us the 
simplest course to attack the metal surface by means of chemical 
reagents, and to see if it has changed its properties in consequence 


683 


of this. If a metal really contains different kinds of ions they will, 
as was stated before, differ in reactive power; hence an attack may 
result in a change of the concentration in the metal surface, in the 
sense of enobling. It is, however, to be seen beforehand that the 
investigation in this direction will be successful only when the in- 
ternal equilibrium in the metal surface in contact with the electro- 
lyte is established slowly enough. If this equilibrium is established 
with very great velocity, no disturbance will of course, take place, 
even though the ion-kinds differ greatly in reactivity. 

It appeared in our previous investigation about polarisation that 
the metals Ag, Ca, Pb are exceedingly little polarisable, from which 
we inferred that these metals quickly assume internal equilibrium. 
Hence the etching of these metals promised little success. Quite in 
agreement with our anticipations it appeared that the potential dif- 
ference metal- */,, norm. salt solution was not to be changed 
for these metals by previous etching. 

To examine this the electrode of the metal that was to be investi- 
gated, fastened to a platinum thread was etched with acid, and then 
quickly rinsed with water. Then this electrode was immerged in 
a ‘/,, norm. salt solution, and made to rotate, after which the 
potential with respect to a ‘/,, N. calomel-electrode was measured 
as quickly as possible. 


When the above mentioned metals according to our anticipations 
had yielded a negative result, the metals Co, Ni, Cr, and Fe were 
examined with the following result: 


| 


Metal | Potential rise through etching 
| by HCl 0,108 V 
Co | 5 abSoy 0,109 ,, 
| » HNO; 0,107 ,, 
by HCl 0,04 V 
Ni » HNO; 0,10 5, 


» Br-water 0,00 ,, 


by HNO; 1,00 V 
Gr , Br-water 0,60 ,, 


Fe by HNO3 above 1,00 V 


684 


It follows from this table that these metals about which it was 
derived from the phenomenon of polarisation that they assume their 
internal equilibrium much more slowly than Ag ete. really become 
nobler when etched with acid, as was expected. 

This temporary change of the potential difference in the sense 
noble must find its origin in a change in the metal surface, and so 
it is perfectly clear that theories 3,4, cannot be of any use here. 

At the same time they throw a peculiar light on Grave’s theory. 
Grave thinks that the heterogeneous equilibrium metal-electrolyte 
can be easily retarded, but that the hydrogen exerts a positively 
catalytic influence on the heterogeneous equilibrium. According to 
him iron would become passive by extraction of the dissolved hydrogen, 
which would take place on anodic polarisation. Now specially in 
ion-state hydrogen is certainly a catalyst for the transition passive 
— active, but it is quite unpermissible to derive from this that 
hydrogen catalyses the heterogeneous equilibrium. It is of importance 
to state emphatically that according to Gravr’s theory it could by 
no means be expected that an enobling of the metal surface would 
be brought about when it was etched with HCl or H,SO,, in which 
the metal can absorb hydrogen. We have to do here with a pheno- 
menon that cannot be counteracted by the positively catalytic influence 
of the hydrogen on the internal transformations in the metal surface. 

Further we made the following in our opinion very important 
experiment with iron. An iron electrode forged to a platinum wire 
was made passive one time through anodic polarisation, another 
time through immersion in strong nitrie acid. Both times the potential 
of these passive states of the iron electrode immerged in */,, N.FeSO, 
solution, was measured with respect to */,, norm. calomel, in which 
the following appeared. 

The potential difference of the passive iron, both after anodic 
polarisation and after etching with strong HNO, at first decreases pretty 
rapidly, then remains constant for a time, and then descends again 
rapidly. We now compared the temporarily constant potential differ- 
ence of the quickly rotating electrode in the two cases, and then 
found what follows: 


Tension of the constant part of 


OSEEN OIE the potential of passive iron 
Passivity arisen by anodic polari- -+0,20 V with respect to 1);9 Norm. 
sation Calomel electrode 


Passivity arisen on attack of -+-0,205 V with respect to*!/;9 Norm, 
strong HNO; Calomel electrode 


685 


From this experiment the important conclusion could, therefore, 
be drawn that the two passive states are the same. 

At the end of this series of experiments we may finally already 
conclude that from the fact that where anodic enobling was observed, 
also ore enobling could be demonstrated, follows that the two 
phenomena must be explained from one and the same point of view, 
as the theory of allotropy makes possible. 


2. As the course followed bade fair to lead to success, we have 
changed our mode of procedure so that we could expect still greater 
effects. 

Our purpose was now to attack the metals while they were im- 
merged in the salt-solutions, and measure the potential with respect 
to the calomel-electrodes at the same time. 

Very effective in this respect is bromic water, with which in some 
cases enormous effects were obtained, and a catalytic influence was 
also discovered of Br-ions for Ni. 


Nickel. 


The first experiment was made with a screwshaped Ni-electrode, 
which was kept in rapidly rotatory mction by a motor, and served 
therefore at the same time as stirrer. The result was as follows. 


Ni-electrode in 100 cm$ '/,;g N. Ni(NO3)9-Solution. 


| 


| Potential of the Ni-electrode with 


Observations | respect to !/;) Norm.Calomel-electrode 
Initial value + 0,15 V 
with one drop of Br-water + 0,44 , 
pO GrOps!) iy, -) + 0,51 , 
5 7 * + 0,64 ,, 
eel is 7 7 + 0,67 , 
5 8 ene 5 3 + 0,80 , 
Now a pretty abrupt descent of 


the potential set in. 
| After 4 minutes the potential is 
constant 
+ 0,42 V 


At last 2 drops of pure Br. are ) 
added i) qr URE 


686 


It follows from this table in the first place that addition of bromic 
water makes the potential of the nickel rise at first by about 0,65 Volt. 
Then a maximum is reached, after which a considerable decrease 
takes place. We further see that when after the potential did not 
change any more, the bromic concentration was raised to saturation 
by the addition of three drops of bromine, the potential of the Ni 
changed only exceedingly little. 

This very remarbable result’) led us to suspect that the disturb- 
ance of the internal equilibrium caused by the action of the bromine, 
is catalytically influenced by Br’-ions which had arisen when the 
metal was etched. With certain Br’-ion-concentration the positive cata- 
lytic action of the Br’-ions is so great that it can just compensate the 
disturbing action of the bromine, and the br’-ion-concentration increasing - 
continually, a considerable decrease will then have to set in. If now 
the bromine concentration is increased considerably, both the disturb- 
ing action and the catalytic action is greatly increased, after which 
ihe condition can become pretty well stationary, and addition of 
more bromine has litthke or no influence. To test this supposition 
the potential of the Ni was first carried up by bromine water, and 
then KBr was added with the following result : 


Ni-electrode in 100 cm3 !/;9 Norm. Ni(NO3)2-solution. 


| Potential of the Ni-electrode with 


Observations | respectto !);9 Norm. Calomel-electrode 
Initial state | + 0,07 V 
With 5 drops of Br-water + 0,52 ,, 
Bo OMe eke H + 0,64 , 
» 2 cm? N.KBr solution + 0,24 ,, 
» 2 drops of pure Br + 0,35) ,, 
After this a slight decrease takes 


slowly place. 


We see from this that addition of KBr made the potential of Ni 
really decrease greatly, but then it was necessary in order to get 
more certainty about the signification of the phenomenon to examine 
in how far Ni behaved here as a Bromine electrode. 


‘) The same result was oblained with a Ni-electrode glowed in vacuo, from 
which follows that possibly dissolved hydrogen exerts no influence on the pheno- 
menon. 


687 


For this purpose besides a Ni-electrode, also a_ Pt-electrode 
covered with Pt-black was placed in the same Ni-nitrate-solution, 
and then after addition of Br-water the potential of the Ni- and of 
the Bromine-electrode was determined. 

Then the following was found : 


Ni and Pt-electrodes immerged in 100 cm3 N. Ni (NO3)9-solution. 


7 oe 


Potential of the Br-elec- 


| Potential of the Ni-elec- 


Observations | trode with respect to | trode with respect to 
igN. Calomel electrode 119 N. Calomel electrode 
Initial value (Key ES | == 0105) Vane 
| 5 €0,60V, > 085 v 
With 10 drops of Br-water + 0,27 , | + 0,82',, 
= ost | S002 
” 1 cms Ue ae 8) | ile 0,58 ” | =F 0,84 ” 
| > 004. | SSH 
a Sp ” ” = 0,62 , | + 0)83) ;, 
>—0,16 , > — 0,04 , 
» 1, N.KBr-solution | + 0,46 ,, + 0,79 , 
005i 101040" 
” 4 n »” ” aly 0,41 ” ar 0,75 ” 
| SSG | SSO. 
9 es »Na-thiosulphate| — 0,43 , i == 0,04; 
| 


Of an unassailable metal which behaves as bromine electrode it 
may be expected according to the formula : 
V Cai, 
Vinet. — Veo. = A=A, + 9,058 log’? ———= 
C By! 
that the addition of the first small quantity of bromine will give 
rise to a considerable increase of the potential difference, while a 
subsequent increase of the bromine concentration must exercise a 
much smaller influence. Our bromine electrode very clearly exhibited 
this behaviour ; the first 10 drops of brominewater made the potential 
rise 0,85 Volt, whereas the subsequent addition of 1 em* resp. 3 em* 
of bromine water no longer practically changed the potential. 
Increase of the br’-ion-concentration must lower the potential differ- 
ence of the bromine electrodes again, and this too was observed. 
By the addition of 1 cm’® of N.KBr-solution the potential fell 0.04 
Volt. That this lowering is not greater is owing to this that during 
the action of Bromine on nickel bromine ions had already been 
formed. 
In conelusion we removed all the bromine by addition of Na- 


1) This negative value must be attributed to the catalytic influence exerted by 
KBr in the preceding experiment. 


688 


thiosulphate, and then the potential fell to — 0,04 V., which was 
about the initial value. If we now compare the behaviour of the 
Ni-electrode with this behaviour, we notice that the addition of the 
fist quantity of bromine has a smaller influence than for the bromine- 
electrode, and that the addition of more bromine has a much greater 
influence here than for the bromine-electrode. 

While the potential of the bromine electrode no longer changes 
on further addition of Bromine up to 3 em*., it increased for the 
nickel-electrode by an amount of 0,384 V., so that the total rise 
amounted to 0,95 V. 

And we see further that while the addition of KBr brought about 
a decrease of only 0,04 V. for the bromine-electrode, it came to 
four times the amount, viz. to 0,16 V. for the nickel-electrode. 

All this suggests that the nickel-electrode does not behave at all 
as a bromine-electrode in the experiments mentioned here, which is, 
indeed, not astonishing, as the br pretty strongly attacks the Ni-electrode. 

It is, therefore, clear that we have to do here with a very parti- 
cular behaviour of the metal itself, and that the explanation, as was 
already surmised, must be this that during the action of bromine 
on nickel a disturbance of the internal equilibrium takes place in 
the meta! surface, in the nobler sense, and that this disturbance is 
counteracted by addition of Br-ions, from which follows that bromine 
ions execute a positively catalytic action. The result is that we have 
observed bere a great disturbance of the internal equilibrium in the 
metal surface caused by chemical action, which proceeds continuously, 
in the same direction as was found in case of anodic polarisation. 
The electrolytical solution of metals is, however, very certainly the 
most efficient means to disturb the internal equilibrium in the metal, 
and thus in this way an anodic polarisation of 1,88 V. was observed 
for Ni, which after the current had been broken off still amounted 
to 0,95 V., a value which is in fairly good agreement with that 
found now. The disturbance brought about by Br during the rinsing 
of the electrode with water being again neutralized, the previous 
etching experiments with Br had a negative result. 


Chromium. 


Of all the metals which we have investigated up to now, chro- 
mium is nearest akin to Ni. 

The following table represents the result obtained when bromine 
was added to a rotating chromiumelectrode immerged in a ‘/,, 
N.CrCl,-solution. 


689 


Cr-electrode in 100 cm3 1/;9 norm. CrCl,-solution. 


Potential of the Cr-electrode with 


Observations | respect to !/;9 norm. Calomelelectrode 
Initial state with active chromium!) | — 0,26 V 
with 3 drops of Br-water — 0,08 ,, 
then slowly descends to 
—- 0,24 V 
with 1 cm3 of Br-water + 0,62 , 
rises in a few minutes to 
-++ 0,79 V 
with 2 cm3 of Br-water + 0,79 , 
with | cms of N. KBr solution + 0,78 , 


Then the preceding experiment was repeated with a solution of 
Cr(NO,), with the following result : 


Potential of the Cr-electrode with 


Observations respect to '/;) Norm. Calomelelectrode 
Initial state — 0,35 V 
with 9 drops of Br-water + 0,73 ,, 
» 1 cm of N. KBr-solution + 0,74 , 


In the first place we see from this that the chromium elecirode 
undergoes an exceedingly strong enobling, in which the metal beco- 
mes passive, as could be demonstrated. By 1 cm’. of bromine water 
the potential rises more than 1 Volt. Further we see that addition 
of KBr has no influence on the Cr-potential, which proves both 
that chromium does not behave here as bromine electrode, and 
that Br'-ions do not exert a catalytic influence on the setting in of 
the metal equilibrium. The metals Co, Al gave a smaller rise of the 
potential when attacked by Bromine. 

We shall revert to this behaviour later on. 


1) The commercial chromium is passive, and can as Hrrrorr states, be activated 
by heating with strong HCl, Z. f. phys. Chem, 25, 729 (1898) and 30, 481 (1889), 


690 
Tron. 


The metal iron yielded a remarkable result. The potential of a 
rotating iron electrode immerged in 100 em*. of '/,, NFeCl’, could 
be ajjected neither by addition of bromine up to saturation, nor by 
addition of a solution of N.KBr. 

This remarkable result must be explained in the following way. 
As we. shall soon see, iron is strongly attacked by a solution of 
FeCl,, and when acted on in this way iron becomes nobler. Now 
Br. also attacks iron pretty strongly, and this attack would undoubt- 
edly also lead to an enobling of the iron surface. Evidently, how- 
ever, the disturbance called forth on attack by Br, is slighter than 
that caused by FeCl,, on account of which the addition of Br could. 
of course have no influence in the just mentioned experiment. What 
is further most convineingly proved here is this that the iron abso- 
Jutely cannot behave as bromine electrode in consequence of the attack. 

This is quite in accordance with what has now been found by 
us, that namely an enobling of the potential of a metal-electrode 
caused by addition of bromine, must be attributed to a disturbance 
of the internal metal equilibrium, at least when the metal is attacked 
by bromine. 

Chlorine acting more strongly on iron than bromine, it was 
expected that when the former experiment was repeated with chlo- 
rine instead of with bromine, a marked rise of the iron potential 
would be found. As the following table shows, this was actually 
the case. 

Fe-electrode in 100 cm3 of N.FeCl3-solution. 


a ST 


Potential of the Fe-electrode with 
| respectto !/;9 Norm. Calomel electrode 


Observations 


Fe in Norm. FeCl3-solution — 0,292 V 
> 0,108 V 
In a current of chlorine. — 0,184 , 


We may be sure that the iron which is strongly attacked by 
chlorine, cannot have behaved here as chlorine electrode, and that 
this experiment therefore proves that we have succeeded also for 
iron in disturbing the internal equilibrium in the surface. 

Another phenomenon which is in perfect harmony with this view, 
and which had already been observed by FINKELSTEIN *), is the elec- 


1) Z. f. phys. Chem. 39, 91 (1901). 
phy 


691 


tromotive behaviour of iron with respect to solutions containing a 
varying ferro- and ferri-ion content, as appears from the following 
table. 

ferrosalt 


Fe-electrode in solutions with varying ratio RSRGISEIE: 


| Potential of the Fe-electrode with 


Obseqvation | respect to 1/19 of N. Calomel electrode 


Fe-electrode in 1 N. Ferrosulphate | — 0,622 V 
» YN. Ferro + 14N. 
Ferrisalt — 0,400 ,, 
in 1 N. Ferrisulphate | — 0,292 ,, 


As was said in the introduction, the complexity must first be 
proved, and then we may try and decide whether the ions differ 
in valence. 

The theory of allotropy already considered the anodic polarisation 
phenomenon of iron a clear experimental proof, and now the attack 
experiments have furnished in our opinion the first irrefutable proof. 

And now that this stage is reached the electromotive behaviour 
of iron with respect to solutions with varying ferro- and ferri-ion 
content appears in a new light. 

Now that we namely know that iron must contain different metal 
ions, it was natural to try it 
the observed phenomena may 
be accounted for from the new 
point of view on the assump- 
tion that iron contains ions_ of 


different valence. And_ really, 
for so far as we can now sur- 
vey the region of the observa- 
tions, this attempt is entirely 
successful. ‘. 

If we construct a A,wx tigure 
for the system Fe-electrolyte in 
the way as was already indi- 
eated by one of us, the con- 
nection between the pseudo-bi- 


nary and the unary system 
drawn in fig. 1 harmonizes well 


with the experimental facts. 
The stable unary electromotive two-phase equilibrium is indicated 


692 


by the solution / and the solid phase S. This solid phase, therefore, 
contains very much of the less noble pseudo component a. The 
metastable unary electromotive two-phase equilibrium is indicated 
by the solution ZL’ and the solid phase S’, 

As was set forth before, on anodic polarisation the metal phase S 
will move down along Sd, hence become nobler, whereas the metal 
surface will move upward along Sa on cathodic polarisation, hence 
become less noble. 

The stable unary electromotive equilibrium requires an electrolyte 
which contains only exceedingly few ferri-ions (?) by the side of 
the ferro-ions («). When iron is immerged in a solution of ferri- 
chloride, the system tends to assume unary electromotive equilibrium, 
in which we may assume the metal phase to send ferro-ions into 
solution, whereas ferri-ions are deposited from the solution on the 
metal. 

As follows from the A, v-figure, a solution containing many ferri- 
ions could only be in pseudo-electromotive equilibrium with the iron 
for much less negative potential of the iron. Hence there will be a 
tendency to make the electrolyte richer in ferro-ions, and the metal 
in ferri-ions, but until the unary equilibrium concentration has been 
reached, the iron potential will possess a too small negative value, 
as was also observed. 

It is further to be seen that the negative value of the iron poten- 
tial will have to increase in a solution of ferro-sulphate, when 
during the measurement the ferri-ions are precipitated as much as 
possible. 

This follows, indeed, from the following table. 


Initial potential of Fe in }/;g N. FeSO4-solution ') = — 0,538 V 

Potential - idem . with a little NH,CNS =—0,578,, 
” ” idem Uy Ue oy HPO, = — 0,569 ” 
= . idem » » » NH,oxalate=—0,555,, 


The removal of the ferri-ions makes the iron clearly baser. 

It is here the place to point out that in the just mentioned etching 
experiments with chlorine, this substance has only indirectly caused 
etching. It is namely very well possible that the action of the 
chlorine has consisted in this that the ferro-ion emitted by the iron 
is immediately converted into the ferri-ion, in consequence of which 
the electrolyte remains as far as_ possible from the concentration 
of the unary electromotive equilibrium, and that this gives to 
the electrolyte its maximum etching action with respect to the iron 
electrode. 


1) This solution contained traces of ferri salt. 


693 


In this case the chlorine would, therefore, indirectly bring about 
an inerease of the disturbance of the internal equilibrium. What is 
not improbable for iron, may also be true for nickel in the experi- 
ment with bromine, when namely the nickel possesses ions of 
different valence, but this cannot yet be stated with certainty. 

Besides this figure accounts for the discontinuous course of the 
potential, when passive iron immerged in an iron-salt solution, passes 
into the active form. 

Iron which has passed into the passive state by anodic polarisation 
or by attack with strong HNO,, is greatly enobled superficially, and 
the potential possesses even a positive value. The concentration of 
the surface of passive iron, therefore, corresponds to a point on the 
line eb, and that below the line A= 0. 

When this passive iron is immerged in a solution of ferro-sulphate, 
transformations will take place, in consequence of which the unary 
electromotive equilibrium is approached, and while the potential is 
falling, the metal surface moves upward along /e, till it has arrived 
in e. Here a second metal phase must occur, viz. d, and as long 
as the two metal phases occur side by side, the potential of the 
metal remains constant. The phase e must be entirely converted to 
d, and when this has taken place, the potential descends further, 
till the unary electromotive equilibrium has been reached, and the 
metal phase has been superficially transformed into S. 

This is exactly the behaviour that has been observed by many 
others and also by us. According to our measurements the three- 
phase equilibrium cde must lie at + 0,20 V. with respect to */,, N. 
calomel electrode. The place of the dotted line 4 =O is therefore 
not correct here; it must be thought between ZS and cde. 

We too found that the transition passive-active is accelerated by 
H-ions, and we are therefore obliged to assume that hydrogen is an 
accelerator for the internal transformations in the metal, as are also 
the ions of the halogens. On treatment with strong HNO, and on 
anodie polarisation the hydrogen is superficially removed, and this 
greatly promotes the internal transformation, so that the strongly 
metastable state which we call passive iron, is observed for some time. 

Through the diffusion of the hydrogen from within towards the 
surface the passive iron, no longer subjected to the action of strong 
HNO, or anodic polarisation, will soon again return to the active 
form. 

Summarizing we come to the following conclusion. 

1. Farapay’s oxide theory, which seemed already sufficiently 
refuted by others, cannot give an explanation of the origin of the 


694 


passivity. If a metal is once passive, it can undoubtedly be covered 
by an oxide coat on anodic polarisation, but the formation of this 
coat is a secondary phenomenon. 

Leaving apart whether on anodic polarisation oxygen charges 
give rise to a certain rise of the potential, it should be borne in 
mind that it is exactly the origin of these gas charges that is to be 
explained. Only when the metal during the passage of the current 
undergoes. a rise of the potential and the tension of generation of 
the O, is reached, these gas charges can arise, and so a theory 
which purposes to explain the phenomenon of passivity, will have 
to account for this potential rise. 

lt follows from this that the theories of FrepkENHacen, MutrHMANN, 
FRAUENBERGER and others leave the essential part of the passivity 
phenomenon an open question. 

3. Our experiments have proved that the phenomenon of 
passivity resides in the metal itself, and that though this phenomenon 
is decidedly a phenomenon of retardation, this retardation is not a 
retardation of the ion hydratation in the electrolyte, as Le Brane 
thinks, but a retardation of the ion transformations in the metal- 
surface. 

4. It is perfectly true, as Grave states, that hydrogen accelerates 
the setting in of the electromotive equilibrium. That the hydrogen 
would accelerate the setting in of the heterogeneous equilibrium metal- 
electrolyte, 1s an untenable supposition. 

The hydrogen accelerates the establishment of the homogeneous 
internal equilibrium, but has often appeared to be inadequate to 
neutralize the disturbance of the equilibrium brought about by etching. 

5. With regard to Finkeisrein’s (Kriienr’s) view it might be said 
to be impled in the new conceptions to which the theory of allo- 
tropy has led, but that the said observers, not understanding the 
deeper signification and the drift of their assumption, were not 
able to embody tneir view in a theory. 

6. W. J. Miier’s views, which are only distinguished from 
those of FINKELSTEIN (KriGER) by the assumption that the states of 
different valence formed different phases, are theoretically incorrect, 
and have therefore not led to any result either. 

7. The trustworthy experimental data about passivity mentioned 
in the literature, just as the new results in this department described 
here, can all be easily explained by the application of the theory of 
allotropy to the electromotive equilibria. 

Anorg. Chem. Lab. of the University. 
Amsterdam, Sept. 25, 1914. 


695 


Chemistry. — “On gas equilibria, and a test of Prot. van pnt 
Waats Jros formula.” I. By Dr. F. E. C. Scoerrer. (Communi- 


eated by Prof. J. D. vAN per Waats). 
(Communicated in the meeting of Sept. 26, 1914). 


1. Introduction. 


It may be supposed as known that the situation of the equilibrium 
of a gas reaction at a definite temperature.can be caleulated, when 
at that temperature we know the energy of reaction and the variation 
in entropy free from concentration for molecular conversion according 
to the chemical equation of reaction. Both quantities are algebraic 
sums of the energies and entropies of the reacting gases separately, 
in which the terms referring to substances of different members of 
the equation of reaction have opposite signs. Energy and entropy 
of a gas free from concentration are pure functions of the tempe- 
rature ; in the expression for the “equilibrium constant” as funetion 
of the temperature the transformation energy and the change in entropy 
free from concentration at one definite temperature and the tem- 
perature coefficients of both occur as constants. The transformation 
energy of a great number of reactions may be directly derived from 
BertHeLor and THomsen’s tables; the temperature coefficients are in 
simple relation with the specific heats, and for this a great number 
of data are found in the literature; the transformation entropy, how- 
ever, is generally not determined directly, but from the chemical 
equilibria by the aid of the above expression. 

If one purposes to calculate the chemical equilibria from caloric 
data, one will have to apply instead of the said mode of calculation 
of the transformation entropy either direct determinations, or another 
mode of calculation, in which exclusively quantities of the gases 
separately are used. The determination of electromotive forces of gas 
cells might be counted among the direct measurements ; for the tem- 
perature coefficient of the electromotive force is a measure for the 
transformation entropy. But this method cannot be applied for a 
great number of reactions e.g. for dissociations in molecules or atoms 
of the same kind. 

Hence the calculation of chemical equilibria will succeed only when 
we have a method at our disposal to calculate the entropies of the 
gases separately or the algebraic sum of the entropies of a gas equi- 
librium from the constants of the substances. 

The thermodynamic entropy of a gas is a quantity, which through 
its definition is determined except for a constant, and it is therefore 

46 

Proceedings Royal Acad. Amsterdam. Vol. XVII. 


696 


clear that the above mentioned calculations of the entropy of the 
gases separately have only sense for another definition of entropy. 
If the entropy is defined as a function of the probability of the con- 
dition, it is possible to find a definite value for this entropy ; but 
this value will vary with different meaning of the “probability”. 
Thus the expressions derived by Kerrsom'), TreTropr *), and Sackur *) 
for the entropy of gases present differences which are the consequence 
of different definitions of probability. These differences only oceur in 
the constant part; if these differences cancelled each other in the 
algebraic sum, a test by the equilibrium determinations could not 
give a decision about the correctness of the entropy values. When, 
however, the algebraic sum of the entropies according to SACKUR 
and Trrropr are drawn up, it appears that these differences continue 
to exist also in the algebraic sums, and it must therefore be possible 
from experimental determinations at least if the accuracy is great 
enough to get a decision which expression is correct. 

While these calculations yield a value for the entropy of the 
gases separately, Prof. vaAN per Waats Jr. has derived an expression 
for the “equilibrium constant” of gas reactions, from which the 
algebraic sum of the entropies can be easily derived; the entropy 
of the gases separately is again determined here with the exception 
of a constant. Besides this expression tries to take the variability of 
the specifie heat with the temperature into account‘). I intend to 
test this formula and the above mentioned expressions of Sackur 
and Trrropr by a unmber of data from the chemical literature. 


2. The expressions for the entropy of gases. 


For monatomic gases Kersom, Sackur, and Trrropr give the value 
for the entropy free from concentration (eventually after recaleula- 
tion) successively by the following expressions: 


3 3 5 3 
he 5 Rlrn T + 3 Rin R - : RinN+ 5 Rinm—3Rinh + C, . (1) 
. : . : s a 
in which C, represents according to KeEsom R /n a+ R{ 4-+ in ale A 


: 3 3 
according to SACKUR 5 Rin 2a + R, and according to Trrropr 


1) Keesom. These Proc. XVI, p. 227, 669, XVII, p. 20. 

2) Terrope. Ann. de Phys. (4) 38. 434. 39. 255, (1912). 

8) Saokur. Ann. d. Phys, (4) 86. 958, (1911); 40. 67, 87, (1913). 
4) These Proc. XVI p. 1082. 


697 


3 5 
~f In 20 + ai R.*) This value of ©, amounts successively to 3,567 R, 
_ — 


4,257 R and 5,257 R. 
The values given by Sackur and Trerropr for di-atomic gases, are: 


Hy = —Rln T41—RinR——Rin N+ -Rlnm — 


“ “ ray 


2 


9 7 
—5Rmh+RnM+—Rm2+—Rinx+C,, . . (2) 


a 


x 
o 


in which C, according to Sackur amounts to R, according to 


( 
Trrrope to > R. 
We get for a tri-atomic gas: 


3 
Ay=\= 8 RaT+3RnmR—4RinN + 5 kRinm — 


1 
—§ Rink + = Rin M,M,M,+-6Rn2+5Rna+ C,, . - (8) 


in which C, amounts to 3 R according to Sackur, to 4 R according 
to Trrrope. 

Besides the known values NV and h, the moments of inertia of 
the molecules occur therefore in these expressions. For the di-atomie 
molecules J/ is the moment of inertia of the dumbbell shaped mole- 
cule with respect to an axis through the centre of gravity, normal 
to the bar of the dumbbell; for the tri-atomie molecules J7/,,./, and 
M, are the three chief moments of inertia, which accordingly depend 
on the relative position of the three atoms in the molecule. 

For equilibria in which only mon- or di-atomic molecules parti- 
cipate, the moments of inertia of the di-atomie particles therefore 
occur, which can be approximately calculated from the different 
determinations of the mean molecule radius. For a_ test of the 
formulae by equilibria of tri-atomic molecules, however, a hypothesis 
concerning the relative situation of the atoms is indispensable, which 
is more or less arbitrary, and can make the test less convincing, 


3. The equilibrium ABZ A+ B. 


For the simplest gas equilibrium ABZA-+ 4, in which the 
atoms A and #& ean be of the same or of different kinds, we 


1) In the expressions of Trrrope |.c. the terms with 2 are omitted, which 
seems justified. 


46% 


698 


find for the algebraic sum of the entropies free from concentration 
making use of the expressions of § 2: 

nH, —1 = 2 (=i) monate = (=) aiat. — 

MAMNB 


—— Rinh — 
m4+mBp 


l 1 3 3 
=>5 Rin Li RinR—~ RinN +— Rln 


3 1 
a Rin2 == Rinx—-RinM+C,, 


(’, amounts to '/, R when Sackur’s values are used, to 
*/, R when Terrope’s values are used. 
Sackur and Terrope’s calculations are based on the following 
assumptions for the specific heats: 


in which C 


3 
Comonat: = 2 es ts Cy diat. —= ry RR. 


The value of the transformation energy in its dependence on the 

temperature is therefore given by: 
ys}, SP Oia Soy fades 

In this expression and the following the molecular values 2 of 
the substances of the second member of the chemical reaction equa- 
tion are. always taken positive, those of the first member negative. 

Inserting these values into the expression for A., we find: 

RT In Kp = — YnET=0 — */, RT + T2nH,= — RT, 

in which 27/7, is represented by the above derived expressions. 
We can transform this expression as follows: 


nk T= 1 
nike melee +—mT—inmM+InC,, . . . (4) 
RT 2 
in which 
InC ai (jo OND +- ue Ink — E m2ax+C,; (4a) 
£ 2 m4 + mB 2 2 é 


C, amounting to —1 according to Sackur’s expressions, to 0 according 
o TETRODE. 


4. In the fifth communication on the law of partition of energy 
Prof. van pyr Waats Jr. derives the following equation for the 
dissociation equilibrium of a di-atomic molecule: 


&,—€& — — 


oi as 0 (aa i. ies Mee er ro) 


MA imp a 2 on. Gata Ce 
€, — &, here represents the transformation energy at the absolute 
zero for one particle; n, and n, represent the number of split and 
unsplit molecules per volume unity; hence we get: 


ny 


699 


cae SnET—0 * SnET—o K ie 
Onan Nii Re a Sia 


Equation (5) can, therefore be written in the following form: 


vh 


1 — — 
+ = In T—In MpIn(1—e ) +imC,, . (6) 


SnET=0 


nk, = —— 
n RT 


in which 
is 3 MAMP $ 1 1 : 
nC, = — ln ————__ -— In2Nh + —Ink — —In2x . . (6a) 
f 2 ma+mp - 2 2 
Equation (6) differs from equation (4) in this that in (6) the term 
with » oeeurs, which takes a vibration of the two atoms in the 
molecule into account; equation (6a) quite agrees with (4a), if in 
the latter Trrropr’s value is substituted; Sackur’s value yields a 
unity difference. 


5. The equilibrium J,Z 2J. 

In the chemical literature a series of acenrate observations occur 
of Starck and Bopenstein'); the dissociation constant of iodium 
is given by them in concentrations, i.e. gram molecules per litre. 
The equations (4) and (4a), resp. (6) and (6a) yield for their disso- 
ciation constant : 


vh 
> E; —— 1 = SS x 
ie Kigy a +5 In T—In M + E (: es )| Vin C. @ 


in which log C, = log C, + 3 (according to Trrrope and v. p. Waazs Jr.); 
log C, = log C, + 2,566 (according to Sackur). 
Making use of the values: V = 6.85 107°. (Prrrin), £ = 1.2110—'6, 


127 
h=5.8810—-2’, m4 =mz = ———., we find: 
6.85 1023 
log C, = — 36.313 (according to TerropE and van DER Waats Jr) 
— 36.747 (according to Sackur) . . . . . . . (Va) 


In equation (7) there occur iwo (resp. three) quantities, which can 
be caleulated from the observations: +n Hypo, M (and »). 

As the term with » can only have slight influence on the result, 
we write equation (7) as follows: 


vh 
SS SS 
Sa ere pa ae thy TM Toa tora EE | 
9.303RkRT ' 2 ee oale oa 9 
— 36.313 (resp. — 36.747) . . (8) 


Let us now assume that 4 remains below 20u, which seems justified 


1) Zeitschr. f. Elektrochem. 16, 961 (1910). 


700 


in virtue of the observations of the absorption lines and their influence 
on the specific heats of other gases (see among others BsmnrruM); we 
then find as extremes for the term with pv: 


3.104. 4.86.10—U 
cero and log (1— 207 ) 


Starck and Bopenstein’s observations now yield the following 
table for the terms of 8: 


TABLE I. 


Second member of 8 


t(Cels)|  T Kg 108) log Kg p | term);—90,,) Y2log T| ——_—__—___—_ 
Bc! Sa 4=0 |4=202 
| 
800 | 1073 | 0.129 | 0.111- 4] 0.693-1 | 1.515 | — 30.909 | — 31.216 
900 | 1173 | 0.492 | 0.692—4 | 0.665—1 | 1.535 | — 31.470 | — 31.805 
1000 | 1273 | 1.58 | 0.199-3] 0.630-1 | 1.552 | — 31.960 | — 32.321 
| | | 
1100 | 1373 | 4.36 | 0.6393) 0.615—1 | 1.569 | — 32.383 | — 32.768 
1200 | 1473 | 10.2 | 0.009-2| 0.5911 | 1.584 | 32.738 | — 33.147 


Van per Waats’s equation for 2—=0O and Terrropr’s entropy 
expressions yield, therefore, the values of the seventh column of the 
above table; Sackur’s values always yield 0,4343 less; Van DER WAALS’S 
equation with 2= 204 yields the values of the eighth column. 

If we now write equation 8 in the form: 


=n Eir— 1) 


+ T log Me IEE 2. 4) ON ree (9) 


2.303R° 
we find: 
TABLE II. 
ATC ATC, | ATC. 
y 9 ‘ 9 
: ao) v ( Al ee es ( AT Je ON ( a7 ja 
1073 — 33166 ==336310) | — 33494 
ery | = 19 | = TS8 al 
1173 — 36915 371493 | — 37308 
37-7 | .88.15 | Hea Saad 
1273 — 40685 — 41238 | | — 41145 
STS = 38.2 | | =ege55 
1373 — 44462 — 45058 | | — 44990 | 
— 37.6 | | — 38.0 | | —asaee 
1473 eeAS 22 20a — 48862 | — 48824 
mean — 37.6 | mean-38.05, | mean—38.3 


| | | | 


701 


ry 


It will be clear that the values of ———* represent the values for 


Al 
log M ecaleulated from equation (9). Therefore the value of J 
becomes 10-876 according to Trrropr, 10-359 according to Sackur, 
10-86 according to Van per Waats for 2=0, 10-33 for 2= 204. 

It is clear from the calculation that the variation of 2 from zero 
to 20m does not cause a change in the order of magnitude of J/, 
that therefore the fact that the frequency is unknown yet renders 
the rough calculation of W possible, and that reversely the frequency 
cannot be calculated but from exceedingly accurate observations. 
With the measurements available at present this is not yet possible, 
as appears from table 2. 

If the iodine molecule is represented by two spheres, the masses 
of which are thought concentrated in the centres, and if the distance 
from the centres is d, the moment of inertia with respect to an axis 
through the centre of gravity and normal to the molecule axis is 

a 
2m i) . From this follows for the limits of d: 
10—276, resp. 10-883 — 2 sees a d—=170:10—* resp: 7 10=9 (10) 
: ~ 6.85 1023.4 


a value which as far as the order of magnitude is concerned is in 


satisfactory concordance with the diameter calculations according to 
other methods. 

6. Sackur and Trrrope’s entropy expressions which were used in 
the preceding paragraph are founded on the assumption that the 
specific heats of the gases are independent of the temperature; the 
test of these formulae can therefore only be a rough one.') In the 
expression proposed by Van per WaAats, the variability of the specific 
heats is, however, taken into account. 

According to this expression the transformation energy for the 
iodine dissociation is represented by : 


< = aes Nvh 
SnE = SnE y=) + °/, RI eee (11) 
ekT —] 


Hence the algebraic sum of the specific heats becomes : 
hy 


dSnE 1 hv\? kT 
=== fh — Sh = ——— 


dT 2 


\) A number of calculations of chemical equilibria carried out by the aid of 
his formula are found in Sackur. Ann, d. Phys. (4) 40. 87 (1918), 


702 
The specific heat of the two iodine atoms is 3 FR, that of the 
iodine molecule therefore 


5 , : ‘hy \? ekT 
~ HER (ae eee li. Ti, eae 


The real specific heat of iodine at 300° C. is according to STRECKER 
8.58 — 1.985 = 6.545. If this expression is substituted for (12), the 
equation is satisfied for 2 — cir. 15. If we use this value for equa- 
tion (8), we get in analogy with tables 1 and 2: 


TABLE III. 
Second member | TC 
t(Cels) (v-term), 15, of 8 (709); 15, (e ~a" 
| Aa jell d=15e4 
800 } On7s led — 33406 
| — 38.01 
900 e051 5 BTN — 37207 
| | == 1SRED5 
1000 OWS |) . = Baeep — 41032 
| ; | — 38.35 
1100 0.705—1 — 32.678 — 44867 
— 38.21 
1200 0.684—1 — 33.054 — 48688 
| mean — 38.20 


This value yields for the atomic distance: 
d= 0.82 10-8 cm. 


If this value is compared with that for the mean molecule radius, 
which has been determined in three different ways, it appears that 
the value for the atomie distance as it is found above, is smaller 
than the mean molecule radius. We must derive from this that 
the atom centra in the iodine molecule lie closer together. Remark- 
able is the agreement of the found d-value with that of the atom 
distances, which were calculated by Manprrstoor from the width 


TABLE IV. 
Gas Radius of Inertia 108 
(o@) 0.566 
HCl 0.22 
HBr 0.165 
Jy 0.41 


of the infra-red bands for three gases '). This agreement appears 
from the foregoing table, in which the values of the three first 
mentioned gases are derived from MAnprERsLoor. 

I hope soon to come back to the application of the used expres- 
sions to some other equilibria. 


Postscript. During the correction of the proofs a treatise by 
QO. Stern in the Annalen der Physik of June came under my notice, 
in which an expression is derived which shows close resemblance 
with that of Prof. van per Waats. Application on the iodine 
equilibrium can also here lead to a small moment of inertia, which 
is however considered improbable by Stern. 


Amsterdam, Sept. 1914. Anorg. Chem. Laboratory 
of the University. 
Chemistry. — “Equilibria in the system Pb—S—O, the roasting 


reaction process’. By Prof. W. Reinpers. (Communicated 


by Prof. 5. Hoocrwerrr). 
(Communicated in the meeting of Sept. 26, 1914). 
Introduction. 


1. The manufacture of galena into metallic lead is mostly carried 
out in this manner that the sulphide is first partially roasted and 
the mass then again strongly heated with unchanged or freshly 
added lead sulphide out of contact with air. Lead is then formed 
with evolution of SO,. 

The reactions that take place in this process known under the 
name of “Rostreactionsarbeit” are generally given in the text-books 
as follows: 

PbS + 20, = PbsO, 

2 PbS + 30, = 2 PbO + 2 SO, 
and then: PbS + PbSO, = 2Pb + 2 SO, 

PbS + 2 PbO = 3 Pb + SO, 


1) Manperstoor. Thesis for the Doctorate. Utrecht. 1914. 


704 


For a proper insight into this process and to answer the question 
whether these reactions actually do take place it is necessary to 
study the equilibria between the different phases that may be formed 
therein. 

After various older researches among which deserve to be men- 
tioned those of H. C. Jenkins and E. H. Smita *), a systematic 
research as to these equilibria was carried out some years ago 
by R. Scnenck and W. Rasspacn *). They determined the equilibrium 
pressure of the sulphur dioxide evolved when three of the four 
phases PbS, PbSO,, PbO and Pb are heated together in an evacuated 
tube at 550° to 900°. 

The conelusions which they drew from these measurements as to 
the nature of the equilibria occurring therein could, however, not - 
be correct in many respects. Their idea has in fact been consider- 
ably modified in various. subsequent publications thereon *). But 
even the last concluding articles still contain many contradictions 
so that it is not plain what equilibria they have actually determined 
and which phases are stable in the presence of each other. 

In the following will, therefore, be discussed (1) the different 
equilibria imaginable in this system and (2) the results will be 
communicated of researches which in consequence thereof have been 
carried out conjointly with Dr. F. Gouprisan. 


2. The equilibria between Pb and the compounds PbO, PbS, 
PbSO, and SO, may be considered as those in a system of three 
components, namely Pb, O, and S$. The isotherm for the equilibria 
between the different phases can, then, be indicated by a triangle 
with these components as apexes. (See fig. 1), 

Let us now first suppose that 

a. only the phases Pb, PbS, PbSO,, PbO and SO, are possible 

4. the gaseous phase is pure SO, and the lead phase pure lead. 

In the last supposition we therefore neglect the small amount of 
PbS in the vapour and the solubility of PbS in molten lead; in the 
first supposition no notice is ‘taken of the basic sulphates which 
according to the later researches of Scuenck and RassBacH *) occur 
as intermediate phases between PbSO, and PbO. 

1) Journ. Chem. Soe. 71, 666 (1897). 

2) Ber. d. d. chem. Ges. 40, 2185 (1907). Metallurgie 4, 455, (1907). 

5) Ber. d. d. chem. Ges. 40, 2947 (1907); 41, 2917 (1908). R, ScHenck, Physi- 
kalische Chemie der Metalle. 

4) Ber. d. d, chem. Ges. 41, 2917, (1908). 


705 


Ss We shall see later how the 
deduced equilibria are being mo- 
dified when we drop these sim- 
plifications. 

sy 3. Let us imagine PbS heated 
at constant temperature between 
600° and 800° in an enclosed 


space wherein a limited quan- 
o lity of oxygen is forced. PbS 
30 is then partly converted into 


Fig. 1. PbSO,. 
The two phases will be capable of existing in the presence of each 


S0, 


Pb 


other and in an unchanged condition at a series of temperatures 
and pressures, 

If on lowering the pressure this falls below a certain limit, one 
of the two following reactions will take place 


PhS PhsOs == 2 Ppa Oo SONY ae, ty 
or PbS + 3PpS0,=4Pb0 +480, .... 2) 


In both cases there are formed in addition to the two existing 
solid phases two new phases, namely fused Pb and SO,-gas, or solid 
PbO and SO,-gas. Hence, between these four phases a monovariant 
equilibrium will set in, which, at a constant temperature, is possible 
only at one special pressure. This will be p, or p,. 

Only in a very special case, namely with an eventual transition 
point where the five phases PbS, PbSO,, PbO, Pb, and SO, might 
coexist, p, and p, are equal. As a rule, however, they are not and 
in consequence only one of the two monovariant equilibria can 
be stable. 

For if p, > p, the reaction (1), in the presence of the five phases, 
will take place from the left to the right and the SO, formed act 
on PbO according to equation (2) in the direction <—. Hence, the two 
reactions together result in the following conversion: 


2PbS-+2PbSO, —4Pb +480, 
4S0, +4Pb0 =3PbSO, + PbS 


Pee eEyOMenaep  erasO,. ©... 26 


This transformation takes place until one of the phases of the 
first member of the equation is used up, whilst the other with Pb 


706 


and PbSO, is left. PbS and PbO are, therefore, not capable of 
existing side by side of each other. 

If, conversely p, < p, the different reactions take place in the 
opposite sense and Pb and PbSO, recede from each other. 

Hence, of the phase pairs Pb + PbSO, and PbS + PbO only 
one can be stable, the other forms a metastable equilibrium. 

Here we have a case quite similar to that occurring with reci- 
procal salt pairs where also only one of the two pairs can be stable. 


4. Let us now also consider the two other monovariant equilibria 
which may be assumed to exist with SO,-vapour and which are 
indicated by the equations 


2 PbO + PbS 223.Pb 4: S0) =. ee 
Pb ++ PbSO,=2 PhO'4- SO, ee 


In the case p, >> p,, it follows at once from the incompatibility 
of the phases PbS and PbO that the equilibrium (4) can be stable, 
but not equilibrium (3). 

Moreover, we then must have p, > p, for otherwise after the 
reaction (1) in the direction — might follow the reaction (3) in the 
direction < which reactions might jointly cause the conversion (5) 
in the direction <—, which is in conflict with the premiss. 

Finally we shall have p,<p,, for then the stable equilibrium may 
also be again attained by the reaction (2) in the direction > followed 
by (4) in the direction <—, namely: 


PbS +3 PbSO,—4 PbO + 480, 
480,-+8PbO = 4 Pbh+ 4 Ppso, 


PbS + 4 PbO =4Pb-+ PbSO, 
Hence, we get this result: 
If Pb + PbSO, forms the stable phase pair, then only the mono 
variant equilibria (1) and (4) are stable and p, > p, > p2 > Ps: 
If PLO + PbS form the stable phase pair, all the reactions 
occur in the opposite sense and only the monovariant equilibria (2) 
and (3) are stable, whereas then p, > p. > pi > Ps- 


5. Starting from the mixture of PbS and PbSO, (for instance a 
in fig. 1) we will, on withdrawal of SO, travel either through the 
monovariant equilibria (1) and (4) (region PbS, PbSO,, Pb and region 
PbSO,, Pb, PbO of Fig. 1) or the equilibria (2) and (3) (region 


707 


PbS, PbSO,, PbO and region PbS, PbO, Pb) to finally retain the 
equilibrium Pb-—+ PbS or Pb-+ PbO after eliminating the SO, as 
much as possible. 

Hence, the reactions (1) and (3), which are generally quoted as 
taking place in the roasting reaction process cannot possibly indicate 
both stable equilibria. 

Of the p-T-lines which Scnenck and RossBacn determined by addi- 
tion of “PbSO,, PbS and Pb and of PbS, PbO and Pb one at least 
must, therefore, indicate an instable equilibrium or an equilibrium 
between phases other than those which were brought together in 
the reaction tube. 

We will see later that both equilibria are metastable and that the 
pressure lines recorded by them relate to the equilibrium between 


, 


other phases. 


6. The supposition made in (2) sub @ is not correct. Between 
PbSO, and PbO there still arrive three basic salts as intermediate 
phases, namely PbO.PbSO, , (PbO), PbSO, and (PbO), PbSO,. The 
first of these can be in equilibrium with PbdSO,. 

The four monovariant equilibria mentioned in (3) now become: 


Bhs a eEsOr= UPHELD SOS 9 coin. se ot 
PbS -—- 7 PbSO, = 4 PbO. PbSO, + 4S0,. . . . (2) 
DsPhO PESO: AaPbSi= FED 51805 7-2) Sh 6) 
Pb! sPusOr== 2 ibb@:.PbSO, SO, =." 08! sa 


and the alternative found must read: 

either Pb + PbSO, stable and then p, >p, >p, > p, and only (1) 
and (2) stable, 

or PbS + PbO. PbSO, stable and then p, << p, << py <p, and only (2) 
and (3) stable. 

Experimental. 
(conjointly with Dr. F. Goupriaan). 

7. In order to investigate which of these two phase pairs was 
stable and at the same time to know the SO,-pressure of the stable 
equilibrium, an intimate mixture of PbS and PbSO, (6—8 grams) 
was heated in a porcelain tube connected by means of a ground 
joint with a manometer and an air-pump. 

The lead sulphide was precipitated from a solution of lead acetate 
with H,S and after washing, dried by heating in a current of nitrogen 
at 200°—300°. 

The lead sulphate was precipitated from a solution of lead acetate 
with sulphuric acid and also dried at 300°. 


708 


The mixture was introduced in a porcelain boat. The remaining 
space in the reaction tube was oceupied by a porcelain rod so as 
to render the gas-volume as small as possible and thus to accelerate 
the setting in of the equilibrium as much as possible. 

The heating took place in an electric furnace. The temperature 
was measured with a Pt-PtRh thermocell and a galvanometer. 


8. Although the reacting substances had been previously dried at 
300° there still was evolved, on heating at 500°, in vacuo, a little 
moisture, which condensed in the colder part of the tubes and was 
removed by a repeated evacuation and gentle heating. 

Subsequently the dissociation pressure was measured at different 
pressures between 500°—700". 

The equilibrium set in very rapidly so that when the tempe- 
rature had been raised and more gas began to evolve there 
could generally not be noticed any change in pressure after 20—30 
minutes. Then a further evolution of SO, was caused by a short 
heating at a somewhat higher temperature and after cooling to the 
original temperature the course of the absorption of the SO, was 
recorded. This also took place very rapidly. The equilibrium was 
thus attained from both sides and yielded figures which differed 
from each other at most 2 or 38 m.m. Also the same pressure again 
set in after an evacuation. The equilibrium is, therefore, independent 
of the total composition, which was confirmed by a change in the 
proportions of PbSO, and Pbs. 

The results are contained in table I. (Fig. 2 Curve I). 


TABLE I. 


7 PbSO, on 1 PbS | 5 PbSO, on 1 PbS || 3 PbSO, on 1 PbS 


t D t p | t p 
5820 | 26 604 50 || «590 | 30 
606 56 634 | 100 || 620 2 
630 94.5 || 660 | 185 |) 670 | 999 
655 156 688 346 | 
680 280 


After the tube had been evacuated a few times and a certain 
quantity of the dissociation product might thus have been formed, 


709 


and as it had been shown that always the old equilibrium again set 
in, the oven was allowed to cool and the tube was withdrawn. 

The reaction product was strongly caked and of a lighter colour 
than the original mixture of PbS and PbSO,. Here and there were 
visible granules with a strong metallic lustre so that at first the 
suspicion was raised that lead had formed as a reaction product. 
On closer examination by means of a magnifying glass these granules 
proved to be very beautifully formed crystals of “galena’” which 
had deposited, besides in the reaction mass, also against the porcelain 
boat and the extremity of the porcelain rod. The analysis showed 
this to be perfectly pure PbS, whilst in the reaction product itself 
not a trace of free lead could be detected. 

Hence, no lead has formed so that the reaction product must be 
basic lead sulphate. PbS +- PhO.PbSO, form the stable phase pair, 
Pb + PbSO, the metastable one. 


9. This was confirmed by the following experiment: 

An intimate mixture of PbSO, and finely divided lead scrapings 
in the proportion of 10 PbSO, to 1 Pb was heated in an evacuated 
and sealed tube for 3 hours at 600°. 

The product obtained gave with hydrochloric acid a very distinct 
evolution of H,S. 

A weighed quantity was now heated in a small flask with strong 
hydrochloric acid and the gas expelled collected in an ammoniacal 
solution of hydrogen peroxide. This solution was boiled for a while, 
then acidified, and the resulting H,SO, precipitated as BaSO,. 

Five grams of mixture containing originally 0.380 gram of Pb, 
yielded 0,040 gram of BaSO,, equivalent to 0,041 gram of PbS. 

According to the equation: 


4Pb+ 5PbSO,=+4Pb0.PbSO,+ PbS . . . (5) 


0,142 gram of Pb has been required for this 0.041 gram of PbS. 
Although the lead has not yet entirely disappeared, a considerable 
quantity of the same has been converted into PbS‘). 


10. The pressures observed almost entirely agree with the values 
found by Scuenck and Rasspacu for the mixture of PbS+PbSO,+-Pb 
as well as for PbS + PbSO,-+ PbO. They conclude that the pressures 


1) Afterwards it came to our knowledge that also Jenkins and Smrrtu (l.c. p.691) 
had already made an experiment from which this is shown. They heated a mixture 
of equal molecular quantities of Pb and PbSO, in a porcelain crucible at dull red 
heat for half an hour; from the residual mass could be expelled with HCl 
a quantity of HS corresponding with 1,41°/, of sulpiur. 


(10 


relate to the equilibrium between the first three phases and that the 
second trio is not stable. From the preceding it follows that both 
equilibria are metastable and that the pressures recorded relate to 
the equilibrium PbS, PbSO,, PbO.PbSO,, SO,. 

The fact that the lead present exerts so little influence on the 
equilibrium pressure proves that reaction (4), which should lead to 
a higher pressure p, and the reactions (1) and (3) in the direction 
— which should lower it either compensate each other or, in com- 
parison with the reaction (2) proceed so slowly that they do not 
perceptibly alter the pressure. Probably the more finely divided 
lead is soon converted and the remaining lead, united to larger 
drops, offers such a small surface of attack that it can react but 


very slowly. 


11. When now from the PbS + FbS50, so much SO, has been 
abstracted that all has passed into PbS + PbO.PbSO, the equili- 
brium has become divariant. The residual phases will be capable 
of existing by the order of cach other in a series of pressures < p,. 

If, however, the pressure falls below a definite limit, a third 
condensed phase appears. Two phases are concerned here, namely — 
Pb and (PbO),.PbSO,. 

As noticed in the case PbS + PbSO,, only one of the two can 
be in stable equilibrium with PbS and PbO.PbSO,. 

This depends on which of the phase pairs PbS + (PbO), PbSO, and 
Pb + PbO. PbSO,, which can be converted into each other by 
double decomposition : 


PbS + 5 (PbO), PbSO, 24 Pb + 6 PbO.PbSO,. . . (6) 


is stable. 


12. In order to investigate this an intimate mixture of finely 
divided lead scrapings and basie lead sulphate in the molecular 
proportion of 38:1 was heated for three hours in an evacuated and 
sealed tube at 670°-—680°. 

The PbO. PbSO, had been prepared by the moist process, accord- 
ing to D. Srrémuoim'), by digesting finely powdered PbSO, with a 
1—2°/, NH,-solution. The analysis of the product obtained gave 
84.88°/, PbO, theory for PbO.PbSO, 84,79°/,. 

The heating of the mixture Pb + PbO.PbSO, yielded apparently 
a but little changed product. It gave, however, a slight sulphide 
reaction. Thus it seemed that the mixture selected did net form the 


\) Zeitschr. f. anorg. Chem. 38, 429 (1904). 


711 


stable phase pair. We must, however, consider that the lead phase 
need not be pure Pb, but may contain dissolved PbS and hence 
there exists the possibility that the PbS found was present, not asa 
free phase, but as a solution in the molten Pb. 

The amount of PbS was, therefore, determined quantitatively. 

From two grams of the mixture were obtained 17,4 mg. of BaSO, 
corresponding with 17,8 mg. of PbS. For the formation of 17,8 mg. 
of PbS according to reaction (6) are required 70 mg. of Pb. Before 
the heating 2 grams of the mixture contained 1,082 grams of lead. 
Hence, there remains 1,022 gram of Pb, which in 100 grams contains 
17,8 , 
Pe tO —— 7 orams Of. Elo: 
1022 

From the observations of Frirprich and Leroux?) it follows that 
the lead solution saturated with PbS at 680° contains 2,5°/, PbS. 
Hence the PbS will be present in the heated mixture not as a free 
phase, but as a solution in Pb, and Pb -—+ PbO.PbSO, will form 
the stable phase pair. 


13. This conclusion was further confirmed by the dissociation 
experiments, starting from a mixture of PbS and PbO.PbSO,. 

These experiments were conducted in a manner similar to that 
in the case of PbS and PbSO,. The SO,-evolution started at 680°. 
The equilibrium set in quite as easily as with PbS + PbSO, and 
could be determined readily from both sides. Also, after removal of 
larger quantities of SO,, the same equilibrium pressure was again 
always obtained. In order to prevent fusion the mass was not heated 
above 800°. 

The results obtained are united in table II (Fig. 2, Curve II). 


TABLE II. 

t p 
712 27.5 
740 63 
750 78 
753 87.5 
770 123 
790 233 


1) Metallurgie 2, 536 (1905). 
47 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


749 


These values correspond very well with the pressures found by 
Scuenck and Rasspacn with a similar mixture and with a mixture 
of PbS + PbO which has been heated above 800° and then cooled. 

On opening the apparatus it appeared that the reaction product, 
although not fused, had strongly caked: the porcelain boat was 
strongly attacked and on the rod a sublimate of very beautiful 
PbS-erystals had again deposited. It was not doubtful that the 
reaction mass contained metallic lead; there could be found large, 
soft paper-marking and malleable particles. Finally, it was proved 
by extracting a portion of the reaction product first a few times 
with ammonium acetate and then with lead acetate. All the PbSO, 
and PbO then dissolves. The residue was treated with fuming HNO,, 
which converts the PbS quantitatively into PbSO,. After expelling ~ 
the HNO, and filtering off the PbSO,, any Pb formed eventually as 
Pb(NO,), must be present in the filtrate. 

The filtrate gave a strong lead reaction. The reaction mass thus 
contains metallic lead. 

Hence Pb + PbO.PbSO, are the stable phase pair and the pressures 
measured relate to the reaction : 


2 PhO.PbSO, + 3PbS—=7Pb+580,.... @% 


14. From the above it follows that with a sufficient excess of 
basic lead sulphate the end of reaction (7) will be a mixture of 
PbO .PbSO, and Pb. (In the latter, however, a little PbS will still 
be dissolved). 

This equilibrium is divariant and, on a sufficient reduction of 
pressure, will pass into a monovariant equilibrium. 

The third condensed phase occurring therein cannot be a second 
metallie phase for the solution of PbS in Pb already present is 
mixable with pure lead in every proportion. 

Hence, it must be the basic sulphate (PbO), . PbSO, which follows 
the PbO.PbSO, and the reaction occurring is indicated by the 
following equation : 

Pb -+ 4PbO.PbSO, = 3 (PbO), PbSO, + SO, -. . 296 

The monovariant equilibrium of this reaction will in turn be 
followed by still two other monovariant equilibria wherein occur 
the reactions represented by the equations: 

Pb + 5 (PbO), PbSO, = 4(PbO), PbSO,-4+ S50, . . (9) 
Pb (PbO);PbSO; = 5;PbO 4+ 50, . © = aa) 

In these reactions primary formed lead therefore disappears on 

behalf of PbO until, finally, only Pb + PbO is left. 


713 


15. Pressures appertaining to the first monovariant equilibrium 
were obtained by starting from a mixture of Pb and PbO. PbSO,. 

Not until 700° an evolution of gas was perceptible. The equilibrium 
sets in with much greater difficulty than in the first two cases; 
generally two or three hours were required. Probably this is due 
to the fact that the metal conglomerates and thus offers but a small 
contact surface with the basic salt. It is also very certain, however, 
that the greater vapour tension of the PbS will have strongly promoted 
the setting in of the previous equilibria of which PbS was one of 
the active phases. The equilibrium could again be attained from 
both sides. 

The following pressures were measured (Fig. 2 Curve III) : 


TABLE III. 

t p 
750° 36.5 
771 61 
789 98 


The tube was subsequently evacuated at 789° and the equilibrium 
pressure again determined. This proved to be unchanged. Even on 


350 
300 
250 
200 


150 


100 A 


———— 


500° 600° 700" 800° 


Fig. 2. 
evacuating a second time the pressure reverted to its old value. The 
pressures measured therefore relate toa purely monovariant equilibrium. 


714 


16. Without opening the apparatus the experiments were now 
continued with the same mixture at 789° The tube was, therefore, 
evacuated for the third time and then again a few times and each 
time the equilibrium pressure was again measured. It now appeared 
that the old pressure no longer set in, but that a lower pressure 
was attained and the more so when more SO, had been withdrawn. 
In suecession were found 93, 75, 61, 54, 41, 34, and 28 m.m. 

This different behaviour can be explained in two ways. 

1. The equilibrium is no longer monovariant, but divariant. Instead 
of three solid phases there are only two, one of which possesses a 
variable composition. This phase might be a very basic sulphate 
with a variable content in PbO. The fusion diagram PbO — PbSO, 
of Scuenck and Rasspacn gives, however, but little support to this ~ 
conception. 

2. The pressures measured are not true equilibria pressures, but 
indicate a stationary condition. 

For if, on evacuating, the pressure falls below the equilibrium 
pressure of equibrium (9) the basie sulfate (PbO), PbSO, can decom- 
pose still further and give rise to the formation of (PbO), PbSO, . 
Pb + PbO. PbSO, then strive, according to reaction (8) towards the 
pressure p,, (PbO), PbSO, + SO, according to reaction (9), however, 
in the direction — towards p,. And when finally both reactions 
take place with equal velocity, we obtain an apparent equilibrium 
at a pressure between p, and p, and dependent on the quantities 
of the different phases. 

It is even possible that PbO is also formed and that reaction (10) 
thus takes place simultaneously. 


17. The second assumption was the most probable one. In order 
to test it more closely a mixture of Pb and (PbO), PbSO, was heated 
in the pressure tube. From this mixture PbO only can be formed 
as the third phase so that only one reaction, that of the monovariant 
equilibrium (10), should be possible. 

(PbO), . PbSO, was obtained by fusion of 1 PbSO, with more than 
3 PbO. As porcelain is strongly attacked by PbO, the mixture was 
heated in a magnesia boat previously heated and saturated with 
lead oxide. 

The result of the measurement at 780° was p= 23, after evacua- 
tion at the same temperature again 22 m.m., then at 800°, 38 and 
after evacuation successively 30, 22, 16 m.m. Thus no constant 
equilibrium is attained. 

On opening the pressure tube nearly all appeared to have been 


(ailis) 


fused and ran through the boat although the temperature had not 
got above 800°, whereas the eutecticum of PbO and (PbO), . PbSO,, 
according to Scnenck and Rasspacu is at 820°. Probably the MgO is 
attacked by the PbSO,. The want of a suitable material which is 
attacked neither by PbO nor by PbSO, or Pb at this high tempe- 
rature renders a correct determination of dissociation pressures for 
reaction (9) and (10) a matter of great difficulty. 

If we accept the value of 20 mm. at 780° as the correct one for 
the equilibrium (10), the p-7-line for this equilibrium would then 
run as indicated by line V in tig. 2. 

The p-7-line of equilibrium (9) then lies between III and V and 
is indicated schematically in Fig. 2 by line IV. 


18. Although from the preceding it is evident that PbS and PbO 
cannot be coexistent, a few experiments were made nevertheless in 
order to confirm this opinion. 

Scnenck and Rasspacw in all their publications consider the equili- 
brium PbS and PbO to be stable although in their dissociation expe- 
riments it had already been shown that with such a mixture repro- 
duceable pressures were not always obtained, for instance if the 
temperature had been raised to above 800°. They also noticed the 
formation of sulphate, but assume that this can only be formed at 
a high temperature and then remains intact on sudden cooling to 
the dissociation temperatures. 

We have now heated an intimate mixture of PbO + PbS for 
some hours at 600—700° in an evacuated and sealed tube. 

The reaction product perceptibly contained sulphate. This was 
estimated quantitatively by boiling a weighed quantity of the product 
with aqueous sodium hydroxide and then passing CO,. The PbSO, 
present is then converted into PbCO,. After filtering and acidifying 
the filtrate the sulphate was precipitated as BaSO,. A check analysis 
was also made on a portion of the mixture that has not been sub- 
jected to heating, under exactly the same conditions of boiling ete. 


Mixture of 4 mols. PvO to 1 mols. PbS. Temperature 670—680’ 
Time of heating 0) lei 3 6 hours 
Gram of BaSQO, per gram of mixture 0,0498 0.0758 0,1000 04121 
Additional sulphate formed on 

heating at 680° 
ingram of BaSO, per gram of mixture — 0.0260  0,0502 0.0623 


If the mixture had been converted completely into basic sulphate 


716 


according to the equation 5 PbO+ PbS = PbO PbSO,-+ 4 Pb, 1 gram 
of the mixture should have yielded 154 mg. of BaSO,. Hence, a 
large proportion of the PbO + PbS has been converted. *) 

The pressures which Scuenck and Rassspacn observed with a mix- 
ture of Pb -+ PbO + PbS do, therefore, probably not relate to an 
equilibrium of these three phases with SO,, but to another equilibrium. 

By a comparison of their observations with our measurements it 
appears that on heating at temperatures below 800° this is the 
equilibrium: Pb + PbO. PbSO, + (PbO), PbSO,, and on heating above 
800° and then cooling, the equilibrium: Pb + PbS + PbO. PbSO,. 

Also below 800° however, this latter equilibrium sets in, which 
with «a sufficient excess of PbS is the most stable, as shown from 
the following experiment: 

A mixture of 4+ mols. of PbO to 1 mol. of PbS was heated in 
a pressure tube. The evolution of gas started at 660°. After evacua- 
tion the following change in pressure was observed at 750°. 


time in min. pressure 

0 5 

7 14 
20 26 
34 33 
42 30 
70 41 
100 44 
160 53 
220 65 
280 74 
340 81 
400 83 
460 83 


The pressure thus rises rapidly to + 38 m.m. and then increases 
gradually to 83. 

The first pressure falls on the p-7-line of Pb + PbO.PbSO, + 
+ (PbO), PbSO,, the second on that of Pb + PbS + PbO.PbSO,. 
_ Similarly was found with a fresh mixture on heating at 790° a 


1) The high result of the sulphate content in the check experiment is very 
striking, because both the PbO and the PbS employed were free from sulphate. 
Evidently the conversion of PbS + PbO into sulphate takes already place at the 
boiling heat in the aqueous solution, from which it follows that also at the 
ordinary temperature PbS and PbO are nol stable in each other’s presence. 


1? 
first halt at + 100 m.m. and then a slow rise io 236 m.m. Both 
pressures are again situated on the above cited p-7Z-lines. 


CONCLUSION. 


19. Summarizing it thus appears that on abstraction of SO, from 
a mixture of PbS and PbSO,, the subjoined monovariant equilibria 
are successively met with, which are indicated in fig. 3 by the regions 


Pelee Tuy IV ‘and: V.. 


PbS—PbSO,—PbO.PbSO, . . . I 
Pb.—PbS—PbO.PbSO, . . . . II 
Pb,—PbO.PbSO,—(PbO),.PbSO, . III 
Pb.—,PbO),.PbSO,—(PbQ),.PbSO, . 1V 
Pba—(PbO),.PbSO,—PbO . . . V 

The lead phase may contain a 
little PbS in solution. As the con- 
tent thereof varies in the different 
equilibria, this difference is repre- 
sented by the indices a, ¢ ete. 
Probably, however this sulphide 
content is very small. 


Ss 


Fig. 2 indicates the pressures 
in these monovariant equilibria 
and the changes thereof with the 


Oo 
temperature. 
Fig. 3. 
Therein region A is the existential region of PbS + PbSO, 
s Lee eBire e 5 » » PbSO, + PbO. PbSO, 
x 3 Coes 7 re »» PbO. PbSO, + Pb 
- a Da, : »  », (PbO), PbSO, + Pb 
3 ee Piney 53 > 95 (PbO), PbSO, ++ Pb 
a Hild ares = 57 DO == Pb: 


Hence, at the temperatures and pressures of region /’ all the 
sulphur will have been expelled from the roasting material. 


20. By substituting the values found in table 1 first series in 
Q 
4,571 T 
thus obtained in pairs, Q, was caleulated for the reaction: 

PbS + 7 PbSO, = 4 PbO. PbSO, + 450, + 4Q, 


the equation log p= — + C and combining the equations 


718 


and as mean value was found — 38390 cals. Applying the same 
principle to the p-Z-values of table 2 we found as the mean value 
for Q, in the reaction: 
3 PbS + 2 PbO.PbSO, = 7 Pb + 5S0, + 5 Q, -— 54324 cal. 
In order to check these, figures we eliminate the unknown heat 
of formation of the basis sulphate from these equations: 
PbS + 7 PbSO, = 4 PbO . PbSO, + 450, — 4 X 38390 cal. 
6 PbS+ 4 PbO. PbSO, = 14 Pb+ 1080, —10 X 543824 cal. 
7 PbS + 7 PbSO, = 14 Pb +1480, —696800cal. 
PbS + PbSO, = 2 Pb + 250, — 99548 eal. 
From the molecular heats ') 
PbSO, = 216210 cal. 
PbS= 18420 ,, 
SO, = 71080 %; 


the calculation for the above reaction at 20° gives — 92470 eal. 
The agreement is tolerable. 


Delft. Inorg. and phys. chem. Laboratory 
Technical University. 


1) LANDOLT. Bornstein, Phys. Chem. Tabelle 1912, 870 and 853. 


(November 27, 1914). 


KONINKLUKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 
of Saturday November 28, 1914. 
Vou. XVII. 


ye 
So 


President: Prof. H. A. Lorentz. 
Secretary: Prof. P. Zeman. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 28 November 1914, Dl. XXIII). 


SL OENE EEE eN a Se 


G. J. Exvias: “On the structure of the absorption lines Dy and D,”. (Communicated by 
Prof. H. Lorentz), p. 720. , 

G. J. Exvias: “On the lowering of the freezing point in consequence of an elastic deformation.} 
(Communicated by Prof. H. A. Lorentz), p. 732. : 

G. J. Exias: “The effect of magnetisation of the electrodes on the electromotive force.” 
(Communicated by Prof. H. A, Lorentz), p. 745. 1 

H. Kameruinen Onnes and G. Ilorsr: “Further experiments with liquid helium. M. Prelimi- 
nary determination of the specific heat and of the thermal conductivity of mercury at 
temperatures obtainable with liquid helium, besides some measurements of thermoelectric 
forces and resistances for the purpose of these investigations”. p. 760. 

F, A. H. Scurememaxers: “Equilibria in ternary systems” XVII, p. 767. | 

F, A. H. Scarememakers and Miss W. C. pe Baar: “On the quaternary system : KC]l— 
CuCl,—BaCl,—H,0”, p. 781. 

T.. S. Ornstems: “On the theory of the string galvanometer of EryrHoven”. (Communicated 

* by Prof. H. A. Lorentz), p. 784. 

L. S. Ornstern and F. Zernike: “Accidental deviations of density and opalescénce at the 
critical point of a single substance”. (Communicated by Prof. H. A. Lorentz), p. 793. 

A. A. Hismays VAN ven Beren and J. J. pk 1a Fontare Scururrer: ‘The identification 
of traces of bilirubin in albuminons fluids” (Communicated by Prof. H. J. Hampurcrer); 
p. 807. (With one plate). 

M. W. Bewerinck : “Gummosis in the fruit of the Almond and the Peachalmond asa process 
of normal life”, p. 810. 

Ernst Conen and W. D. Hetperman: “The allotropy of Lead” I. p. 822. (With one plate). 

J. C. Kivyver: On an integral formala of Strerrses”, p. 829. 

F. E. C. Scurerer: “On unmixing in a binary system for which the three-phase pressure 
is greater than the sum of the vapour tension; of the two components”. (Communicated 
by Prof, J. D. van per WAAts), p. 834. 

Mrs. T. Enrenrest-Aranasssewa: “Contribution to the theory of corresponding states”, 
(Communicated by Prof. H. A. Lorentz), p. 840. 

A. FB. Hotreman: “The nitration of the mixed dihalogen benzenes”, p. 846. 

J. Borsexen and W. D. Conrn: “The reduction of aromatic ketones. III. Contribution to 
the knowledge of the photochemical phenomena” (Communicated by Prof. A. F. Hoiirs- 
MAN), p. 849. 

YP, Enrenrest and H. Kamertincu Onyes: “Simplified deduction of the formula from the theory! 
of combinations which PLANcK usvs as the basis of his radiation-theory, p. 870. 


48 
Proceedings Royal Acad. Amsterdam, Vol. XVII. ; 


720 


Physics. — “On the structure of the absorption lines D, and D,”. 
By Dr. G. J. En1as. (Communicated by Prof. H. A. Lorentz). 


(Communicated in the meeting of April 24, 1914). 


Some time ago Prof. H. A. Lorentz drew my attention to the 
results of an investigation by Miss G. v. Usiscu'). From phenomena 
observed by the writer during the investigation of the polarisation 
state of light emitted by a sodium flame in a magnetic field after 
it had passed through a tube filled with absorbing sodium vapour, 
she infers that the wave length for which the absorption of the 
vapour is a maximum, depends on its temperature, and in such a 
way too that on rise of temperature a displacement towards the 
red takes place. The amount of this at 270° would be about 0.17 A.U. 
with respect to the emission line. If seemed worth while to ascertain 
this result by direct observation. During the summer months of last 
year Dr. W. J. pk Haas and myself occupied ourselves with this question. 

At first we intended to use an échelon-spectroscope for these researches, 
observe by the aid of this the spectrum of a monochromatic source 
of light, and then superpose the absorption lines of sodium vapour 
on this. This vapour was in an iron tube, closed on both ends by 
plates of selected plate glass, and provided with water cooling; in 
the middle the tube, which contained there a vessel of metallic 
sodium, could be heated. Such tubes were used by R. W. Woop 
for the investigation of fluorescence of sodium vapour. First a blow- 
flame served as monochromatic source of light, which was blown 
by means of air in which a very finely divided solution (mist) of 
soda was suspended. Afterwards the flame of a Méker-burner was 
preferred, burning in an atmosphere in which a mist of soda was 
also suspended. This was reached by placing the flame inside an iron 
exit tube, at the bottom of which a reservoir was attached, which 
was in communication with the air, and into which the soda-mist 
was blown by means of an aspirator. This method appeared very 
efficient to obtain a sodium flame of constant intensity, which is 
moreover easy to regulate. : 

The lines obtained by means of this source of light, were too 
broad for the investigation with the échelon-spectroscope when the 
intensity of the light was sufficient for the observation, the self- 
reversal moreover being very troublesome then. If on the other 
hand, the light intensity was diminished till the lines were narrow 
enough, the intensity was again too slight for the observation. 


1) G. y. Usiscu. Inaug. Diss. Strassburg. 1911. Aun. d. Phys, 35. p. 790; 1911, 


724 


We have therefore then tried to see the phenomenon directly by 
means of the spectrometer, which served for provisional dispersion 
in the experiments with the échelon spectroscope. We were of 
opinion that, the dissolving power of the prism system amounting 
to 60.000, it must be possible to observe in this way a displacement 
of the above given amount. Nothing was to be detected of this, 
however. It is true that the at first narrow absorption line (which 
_ has originated by self-reversal in the sodium flame) widened considerably 
on the heating of the Woop tube up to about half the distance of 
the two D-lines, but a displacement could not be perceived. 

On account of Dr. pe Haas’ return to Berlin we had to stop our 
joint observations at this point, and I continued the research alone. 

First I tried to obtain comparatively narrow emission lines, which 
should be intensive enough to superpose the absorption lines on 
them in the investigation with the echelon spectroscope by eleetric 
discharges in a heated evacuated Woop tube with sodium. This, 
however, appeared impossible, the width remained considerable, and 
the self-reversal troublesome. 

Then I took another course, and used an arclamp as source of 
light. To obtain monochromatic light I used the above mentioned 
spectrometer as monochromator, diminishing the widths of the slits 
so that the issuing light comprised a range of only about 0,5 A.U., 
for some observations 0,4 A.U. In this case the adjacent spectra 
will overlap only for a small part, as the distance between two 
successive orders amounts to 0,39 A.U. The dissolving power of 
.the échelon spectroscope, which consists of 80 plates of 14,45 m.m., 
amounts to 450.000 *) for D-light. 

The absorption lines of the are of light, which are caused by 
the sodium vapour present in it, appear, observed in this way, to 
be double. Both for D, and for D, there are two maxima of absorp- 
tion, which are somewhat sharper for D, than for D,, and the 
distance of which is smaller for ), than for D, under for the rest 
the same circumstances. These distances are, however, variable. The 
lamp burning normally, the distance generally amounted to 0.053 
A.U. for D,, to 0.078 A.U. for D, for a point lying in the middle 
of the are, when Sitrmens’ S A-carbons were used. It sometimes 
occurred, however, for a certain pair of carbons that the distance 
was much smaller, down to half the value; sometimes too that it 
was much larger, up to almost double the said amount. When new 


1) The results of the observations made about the components of the mereury 
lines by the aid of Uns échelon spectroscope, were in agreement with those of 
most of the other observers. 


48* 


722 


earbons are set burning, the distance is also much larger than the 
normal one, When the are hisses, the reverse takes place: the lines 
erow fainter, and the distance grows smaller, in case of very decided 
hissing they can even become entirely invisible. Also in different 
places of the are the distance is different, for the negative carbon 
the distance is much larger — about twice as large as a rule — 
than for the positive carbon. 

Between the two absorption maxima lies also a region of absorption, 
which on the whole is of only little greater intensity than the 
maxima of absorption. Now and then it makes the impression that 
there are still more feeble maxima of absorption in this region; I 
have, however, not been able to ascertain this with perfect certainty. 

I could artificially modify the aspect of the absorption lines very 
considerably by blowing a little soda mist into the are by means 
of a tube placed parallel to the positive carbon, which lies horizontal ; 
in order not to disturb the equilibrium of the are the blown in air 
current had to be only very weak, while the quantity of sodium 
could be modified by varying the concentration of the sodium 
solution. It then appeared that always when soda was blown into 
the are the distance of the components of the two D-lines increased, 
these becoming vaguer at the same time. The greater the quantity 
was of the soda that was blown in, the further the components 
were split up, and the less sharp they became. This splitting up 
could even reach an amount of about 0,3 A. U., in which case they 
were, however, very vague. The splitting was always perfectly 
symmetrical with respect to the original double absorption line. The 
maxima of absorption were — for so far as perceptible — of equal 
intensity, the sharpness of the two components also seeming pretty 
well equal. | have not undertaken further quantitative measurements 
about this, since if would have been impossible to determine the 
quantity of sodium in the are, even when the velocity of supply 
was known; at most this quantity could be very roughly estimated ; 
nor was the phenomenon perfectly constant. Similar phenomena, 
still less constant, however, were observed when carbons were used 
which were soaked in a diluted solution of soda. 

When the Woop tube is placed in the way of the rays of light 
so that it follows the spectrometer, which cuts a small portion out 
of the spectrum, so e.g. between object glass and eye-glass of the 
reading glass, the absorption lines of the sodium vapour appear also 
to be double, in which the distance of the components increases as 
the temperature rises. At the same time, however, distinct phenomena 
of anomalous dispersion are perceptible, as soon as the heating of 


723 


the tube takes place in a somewhat unsymmetrical way. For this 
reason, and at the same time on account of the large differences of 
temperature which must necessarily exist in the Woop tube, at 
which there can be no question of saturate vapour, I did not under- 
take quantitative measurements. 

Finally in order to be able to carry out measurements which 
should be liable to interpretation, | have generated the sodium vapour 
in a vertical glass tube, which was first provided with some pieces 
of. sodium, then evacuated down to about O.OOL m.m. of mercury, 
and sealed to. This tube was uniformly heated all over its length 
by an electrical way, so that the temperature may be assumed to 
be the same at all places, and accordingly the sodium vapour to be 
saturate. In the enclosure there were made two apertures, through 
which the light fell in horizontal direction. As the glass gradually 
clouded somewhat at these places, | later on applied side tubes which 
were also electrically heated, while a wider glass tube was also 
used. The bore of the tube, with which | carried out my final 
measurements, amounted to 28 mm. For a reason to be stated later, 
this tube was placed between object glass and eyeglass of the reading 
glass. Of course the image suffered by this, but nevertheless it was 
possible to measure the distances of the components. 

The pbenomena which I observed in this way were qualitatively 
in perfect harmony with what I had seen by means of Woop’s tube. 
and during the blowing in of the soda mist into the are. On vise of 
temperature the distance of the components increases, while they 
become less sharp at the same time. Up to almost 300° the distance 
can be very well measured, the vesults of these measurements have 
been represented in the curves D, and PD,. At higher temperature 
the width is too large to be investigated by means of the échelon 
spectroscope, the phenomenon becoming very vague then, so that 
the absorption maxima are clearly perceptible on slight magnitication 
only, the light intensity is only little greater then between the absorption 
maxima than in the maxima themselves. The greatest width measu- 
red amounts to about 0,21 A.U., as is visible from the figure. 
The resolution is always greater for D, than for D,; the curves 
indicating the course in the two cases run perfectly parallel. On 
the whole the components of D, are somewhat sharper than those 
of D,; of D, the component lying to the side of the red is the 
stronger and sharper, of D,, that which lies to the side of the violet. 
I think I have been able to observe with pretty great certainty that 
the two components of D, are each double, so that the absorption 
region would be bounded here by two absorption maxima on either 


724 


0.05 


° 
200° 250 


side, which can be distinguished from each other with difficulty. I 
have not been able to observe anything similar for D,, there the - 
absorption maxima seemed single to me. At 274° I found about 
0.035 A.U. for the distance of the two absorption maxima, of which 
each component of D, consists, at 290° about 0,045 A.U. The dis: - 
tances of the components of YD, indicated in the figure refer to the 
extreme components. The region lying between the absorption maxima ~ 
situated on either side is on the whole of uniform intensity, whieh, . 
chiefly at tbe higher temperatures, is but very little greater than , 
that of the absorption maxima. Whether there are still more faint 
maxima in this region, I have not been able to observe with certainty, 
though | now and then got the impression that such was, indeed, 
the case, 


725 


In the figure IT have also indicated the mean amount of the width 
of the region of the are absorption by means of short dotted lines. 
Further the curve indicated by p denotes the vapour tension of the 
sodium vapour for the temperature in question. The scale of the 
ordinates on the right hand side of the figure refers to this curve. 
For the determination of this curve I made use of KRONER’S ') research 
on the vapour tension of alkalimetals ; for this it was necessary to 
extrapolate the values found by Kroner, for which purpose I used 
Graitz’s”) formula, which is formed from Dupré-Herrz’s *) formula 
based on that of CLapnyron by assuming the validity of Van pmr 
Waats’s law for the vapour instead of that of Borne-Gay Lussac. 
Grairz’s formula 


ap n 


p-e T — kT—™e GE 

containing four constants, | had to assume four points of the vapour 
tension curve. | took three points for them, which had been directly 
determined for sodium by Kronur, viz. 7= 693, p=2.00 ; T= 733, 
p = 420; T= 773, p= 8.64 (temperatures in absolute scale, pres- 
sures in m.m. of mercury). I derived the fourth point, availing myself 
of Ramsay and Youne’s rule, from Kronur’s determinations for pot- 
assium and found for it 7’= 589, p=0.11. I found from this for 
the constants using Brice’s logarithms, «@ = 28.877, log k = 164.88, 
m = 48.748, n = 18148. By the aid of these constants I calculated 
the values of p given in the figure. 

One might be inclined to ascribe the observed phenomena to ano- 
malous dispersion ; the observed dark lines would then be no absorp- 
tion lines proper, but “dispersion lines”. If this were actually the 
ease, tie light of the considered wave length would only have 
changed its direction, without having undergone absorption. As to 
the absorption lines in the light are, taking the comparatively small 
value of the anomalous dispersion at the densities in question into 
consideration, the point of intersection of the rays of light coming 
from the are with the plane of the spectrometer slit could never be 
far distant from the crater image. When this image is moved over 
the plane of the slit we should therefore have to see light lines in 
some positions instead of dark ones. As I have never observed 
anything like this, not when I placed the are lamp in other positions 


1) A. Kroner. Ann. der Phys. 40. p. 438. 1913. 
2) Grirz. Zeitschr. f. Math. u. Phys. 49 p. 289. 1903. 
8) Herrz Wied. Ann. 17. p. 177. 1882. 
Dupré. Théorie mécanique de la chaleur. p. 69. Paris 1862. 


726 


either, so that the direction of the issuing beam of light with respect 
io the light are was a quite different one, I think I may conclude 
that the are lines are not to be attributed to anomalous dispersion. 

Nor can for analogous reasons this be the ease with the lines 
which were observed after the light’ had passed through sodium 
vapour in a uniformly heated glass tube. Here too light lines would 
have to be observed at some distance from the dark ones, of which 
there was however, no question. 

On the other hand — as I already remarked just now — when 
the unsymmetrically heated Woop tube was used, I saw a sharp 
light line by the side of the dark region, which latter became 
blacker then at the same time; in fact besides the absorbed light, 
also the anomalously dispersed light has vanished from this region. 

Everything considered I am therefore of opinion that anomalous 
dispersion has had no influence on my final results. 

I will mention here another phenomenon, which at first made its 
influence felt in a peculiar way. In my first experiments I had 
placed the glass tubes in which the sodium vapour was generated, 
before the entrance slit of the spectrometer, so that the whole beam 
of white light passed through it. The measurements which I then 
made of the distances of the components for different tubes, which 
were distinguished by the thickness of the radiated layer of vapour, 
were not in harmony; at the same temperature the distance of the 
components was found larger as the radiated layer was thicker. 
This peculiar phenomenon must undoubtedly be a consequence of 
the presence of fluorescence light, which the sodium emits under 
the influence of the incident white light. According to Woop’s 
researches!) it is just the two D-lines which are very prominent 
in the fluorescence light. This light will be the stronger as the 
traversed layer is thicker. In this way it is explicable that the 
absorption spectrum can be subjected to a modification which will 
become greater with increasing thickness of layer. 

When, however, the distance of the absorption maxima increases 
in consequence of the superposition of the fluorescence light over 
the absorption spectrum, which is greatly the case at higher tempe- 
ratures (see the curves (D,)' and (D,)'), it is easy to see that the 
maximum, resp. the maxima, of the fluorescence light must be 
situated between the absorption maxima so that the curve representing 
the intensity of the fluorescence light, exhibits a rise at the place 
of the absorption maxima, when we move to a point lying halfway 


1) R. W. Woop. Phys. Opt. p. 444; 1905, 


727 

between the two absorption maxima, If the absorption maxima 
coincided with maxima of fluorescence, the former wouid either not 
shift their places, or they would split up. Hence we arrive at the 
conclusion that at temperatures above about 260° the maxima of 
absorption do not coincide with maxima of fluorescence, but that 
the latter maxima, resp. maximum, lie between the maxima of 
absorption, 

I have indicated two curves in the figure for which the influence 
of the fluorescence light is visible, the curves (),)' and (D,)'. They 
represent the distance of the components of D, and D, fora radiated 
thickness of layer of 40 m.m., in which the tube of sodium vapour 
was placed before the entrance slit of the spectrometer: the distance 
from the tube to the sht was about 10 em., the opening of the 
incident beam being about L : 10. Under these circumstances it was 
also possible to observe the fluorescence light by means of a spectroscope. 

If the tube with sodium vapour was placed between object glass 
and eye glass of the reading glass, the fluorescence can only be 
brought about by the light that belongs to the narrow spectral range, 
issuing from the spectrometer, instead of through the undivided 
white light. It is easy to see that the part of the fluorescence 
light, which in this case is already very faint, the part that 
finally reaches the retina, will have to be exceedingly small 
in comparison with the observed light; the influence of the 
fluorescence light will, therefore, have to be imperceptible then. I 
have actually convinced myself that when the tube with vapour is 
placed between object glass and eye glass of the reading glass the 
distance of the absorption maxima is independent of the thickness 
of layer traversed by the rays. For this purpose I compared a tube 
of 50 m.m. bore with the tube of 28 m.m. used for the measurements ; 
in these two cases the distance of the components was the same at 
the same temperature. 

I think myself justified in drawing the conclusion from all that 
has been observed that the distance of the absorption maxima of 
the sodium limes is closely connected with the density of the vapour, 
and that in this way that the splitting up increases with increasing 
density. That what has been observed is chiefly an effect of density, 
aud not in the first place a temperature effect, is supported by the 
fact that the influence of the soda mist blown into the are is for 
the greater part the same as that of absorbing sodium vapour of 
much lower temperature. The temperature at which the absorption 
in the are takes place, will namely undoubtedly be much higher 
than that of the vapour in the glass tube. On the other hand the 


phenomenon in the are is dependent in a high degree on the quantity 
of soda, the temperature varying very little as long as the equilibrium 
in the light are is not disturbed. 

In my opinion besides the density also the temperature can have 
influence, though the latter will be slight. If the are lines were 
exclusively dependent on the density of the vapour in the are, the 
horizontal dotted lines in the figure would have to cut the curves 
for D, and D, in points for which the abscissae are equal. As this 
seems to be almost the case, the influence of the temperature cannot 
be very large. 


Also with regard to the degree of the absorption —- so the value 
of the absorption index —, there can very well be difference between 


higher and lower temperatures; I have, however, not examined this. 
And at last, the absorption lines of low temperature are somewhat 
sharper than those in the light are. 

Returning to what Miss v. Usiscu derived from her experiments, 
viz. a displacement of the absorption maxima of sodium vapour on 
change of temperature, we may question whether this result can be 
brought into connection with the observations described just now. 

In the experiments under consideration the main point was the 
absorption to which the components of the two magnetically split 
sodium lines (briefly called ZeEMAN-components) were subjected in 
the Woop tube filled with sodium vapour. 

The measurements were made of the relative intensities of the 
differently polarized beams of light both normal to the lines of force 
of the magnetic field (transversal), and in the direction of the lines 
of force (longitudinal) (in the transversal observations the beams 
polarized parallel to and normal to the lines of force, in the longi- 
tudinal observations both the circularly polarized ones.) These beams 
of light were emitted by a sodium flame which was placed between 
the poles of a magnet: the undispersed sodium light was subjected 
to absorption in a Woop tube. This tube was every time heated to 
a definite temperature, and the temperature being kept constant, 
the magnetic field was varied till the difference of the intensities 
of the differently polarized beams of light was a maximum; this 
measurement took place by rotation of a glass plate, which served 
as a compensator. For every temperature of the Woop tube the field 
was determined, in which the difference of the intensities became a 
maximum. Miss v. Usisch makes the supposition that this difference 
will be a maximum when one ZeeMAN-component coincides with the 
maximum of absorption, and the other is not absorbed at all. By the 
aid of this the writer deduces that at 270° the displacement of the 


729 
° 
sodium lines would amount to 0.47 A.U.; im this ease the differe2&e 
of the intensities was therefore a maximum at a distance of the 


ZEEMAN-components or on an average 0.34 AU. 

Now on closer consideration it is clear that the correct interpreta- 
tion of Miss v. Usiscn’s observations would be very intricate, 
and many more data would have to be available for it. In the 
first place we should have to know the correct distances and 
intensities of the Zenman-components, before they undergo absorption 
in the Woop tube; further the accurate course of the curve that 
denotes the connection between the intensity of the lhght transmitted 
in this tube with the wave length, should be known. The absorption 
maxima of sodium vapour not being sharply defined lines, much 
will depend on the intensity and sharpness of these maxima; this 
is the more obvious when it is borne in mind that the real maxi- 
mum difference of intensity observed by Miss v. Usiscn, constitutes 
only a few percentages of the whole amount. With so small a 
difference we should be sooner inclined to assume a difference 
in absorption to that amount than as the author does, suppose 
that one ZeEMAN-component is not weakened at all, the other 
only a few percentages in the case of a thickness of layer which 
is at any rate pretty considerable. It is easy to imagine cases in 
which the absorption maxima are of equal intensity, but difference 
of intensity of the ZeeMAN-components is a maximum, when they lie 
outside the absorption maxima. 

Everything considered the amount given by the author can only 
represent the distance of the absorption maxima as far as the order 
of magnitude is concerned; accordingly I do not think that the 
result of my observations (distance of the absorption maxima of 
about 0.15 A.U. at 270°) is in contradiction with that of Miss v. 
Uniscu. 

Besides it is possible that the temperature has not been given 
perfectly accurately. In this respect a Woop tube presents more 
sources of errors than the uniformly heated tube which I used. 
Moreover the difference need. not be very great, taking the very 
rapid inerease of the resolution in the neighbourhood of 300° into 
consideration. 

When seeking an explanation of the observed phenomena now that 
it has appeared that in the first place there is here question of a 
density effect, we are naturally led to look for a connection with 
the widening of spectrum lines in general, and with the explanation 
which Stark has given for it, which comes to this that this widening 


730 


would be the consequence of electrical resolutions of the spectrum 
lines. It is easy to understand that the greater the density of an 
(emitting or absorbing) gas, the more frequently it will oecur that 
the vibrating electron systems are in the neighbourhood of electric- 
ally charged systems, and will therefore perform their vibrations 
under the influence of the electric field of these charged systems ; 
hence the spectrum lines brought about by these vibrations will be 
the more perceptible by the side of those which arise from systems 
whieh do not vibrate in an electrical field. In this way we shall be 
able to obtain a great number of lines, which all being superposed, 
can make the impression of a broad band. It is very well 
possible that definite groups of these vibrations can be predominant 
which will give rise to the appearance of maxima of absorption 
(resp. emission). If we wanted to give further particulars about this, 
it would be necessary to enter into an examination of the mechanism 
of the phenomena *). 

As to the order of magnitude of the above described phenomena, 
it is indeed interesting to compare it with the order of magnitude 
of the electrical resolutions as Stark has observed them. When we 
assume that a vibrating system is placed in an electrical field origi- 
nating from an electrical elementary charge at such a distance as 
the mean distance of the atoms in saturate sodium vapour of about 
280° amounts to, the resolution of the D-lines, when taken as an 
electrical resolution, would at this temperature agree as far as 
ihe order of magnitude is concerned — with the resolutions whieh 
Srark found in this part of the spectrum, always on the supposition 
of a linear course of the electrical resolution with the intensity of 
the field. 

Above 260° the observed resolution increases pretty accurately 


with the power ?/, of the density, the increase being slower at the 
lower temperatures ; therefore what was observed just now about 
the order of magnitude of the resolution at 280° cannot possibly 
be of general validity, as this would require an increase not with 
the power */,, but with the power */, of the density. 

I also observed the D-lines in the solar spectrum, which also 
exhibited two components each. On the whole the phenomenon was 
in accordance with what is observed for saturate sodium vapour of 
about 270°. The distance of the components was about 0.15 Nae 


1) Even without thinking of electrical resolutions, | pronounced the opinion 
already before that the “own period” of a vibrating system might vary as 
it was under the influence of neighbouring systems, and that widenings of spectrum 
lines might be the consequence of this. Cf, G. J. Extras, Diss. Utrechit; p. 146 et seq. 


731 


I did not however carry out accurate measurements about this. They 
further seemed to me slightly less sharp than those whieh were 
observed for sodium vapour of low temperature, though this difference 
Was not very conspicuous. If the resolution were really only little 
dependent on the temperature and possible other factors, we might 
draw the conclusion from this that the density of the sodium vapour 
in the chromosphere of the sun is as great as that of saturate sodium 
vapour of about 270°. 

I further made some observations on the emission lines of sodium 
vapour. For this purpose I used a glass discharge tube which con- 
tained some sodium, and which was heated to 200° or 200°. 

It then appeared that. the emission lines, both D, and D,, were 
double, and that the distance of the two light lines increased with 
increasing temperature. It is not impossible that self-reversal plays 
a part in this; it was, however, peculiar in this that chiefly for D,, 
the two light lines on either side of the dark core differed in intensity, 
which would not have to be the case for self-reversal. 

With regard to the emission lines D, and D, Micnetson ') has 
pronounced the opinion that they would each consist of four com- 
ponents, {wo intenser ones, and two very faint ones, the distance 
of the intenser ones amounting to about 0.15 A.U. Fapry and Pxror’) 
are, however, of opinion, that reversal phenomena would play the 
principal part in this. 

In conclusion I will still state that already a long time ago I 
observed for the emission lines of copper when this is in the light 
are, resolutions of entirely the same order of magnitude as those 
which I have now described for the absorption lines D, and D, of 
the sodium, also with the aid of the échelon spectroscope. I then 
observed with a pretty high degree of certainty that these resolutions 
were greater as the density of the copper in the are increased. I 
could not carry out measurements about this, however, as the amount 
of the resolution was very variable, and besides I had no means to 
determine the density of the copper in the are. 


Haarlem, February-April 1914. Physical Laboratory 
of ‘“Tryier’s Stichting.” 


1) A. A. MicHELson and E. W. Moriey. Amer. J. (3) 34. p. 427; 1887. Phil. 
Mag. (5) 24 p. 463. 1887. 

A. A. Micnetson. Rep. Brit. Ass. 1892 p. 170. Phil. Mag. (5) 34 p. 280. 1802. 

2) Gu. Fasry and A. Piror. CG. R. 180 p. 653. 1900. 


Physics. -— ‘On the lowering of the freezing point in consequence 
of an elastic deformation.” By Dr. G. J. Extas. (Communicated 


by Prof. H. A. Lorenz). 


(Communicated in the meeting of May 30, 1914). 


A number of years ago E. Riecky ') derived from thermodynamic 
considerations that a solid body subjected te forces which bring 
about an extension or Compression, will in general exhibit a lowering 
of the freezing point, also at those places of the surface where no 
deformative forces are directly active. 

This case may be extended to that of an arbitrarily deformed body. 

J. Let the free energy per unity of mass be w, and the density @, 
then the total free energy of a certain system will amount to 


v= [ewe eer mol cme 0 (Il) 


in whieh the integration must be extended over all the material 
elements 9.dt. Further we make no suppositions at all on the state 
of the system. 

Let us suppose the system to undergo an infinitely small deform- 
ation at constant temperature. We can always assume this deform- 
ation to consist of the infinitely small dilatations «,, y,, 2:, and the 
distortions y-, 2,2), for whieh the well-known relations hold: 


0g uy 17205 
oa) i ars 
One mnOS 0s § &: Ox ena 2) 
i oa aaa Pea eee a Taee ek IS, 


when §,,§ denote the infinitely small displacements of the points 
of the system. 
In consequence of this deformation the free energy of the material 


element odr will increase by the amount 


Ow Ow 0 ow Ow Ow 
o dt & &y, + ue Yy + wid Ze+ oe yz + - zs fe + eM vy) > (63) 


Oar, 


On the other hand work has been done by the external forces. 
When the components of the joint volume forees which act on the 


1) E. Riecke, Wied, Ann. 54 p. 731. 1895, 


733 


material element odrt are @ Ndr, 9 Vdr, and er, and the components 
of the joint external tensions which act on the surface elements do 
of the surface that bounds the system: p.do, p,de, and p.do, the 
total work of the external forces, the displacements being §, 9, ¢ will 
amount to 


JA = | o (X§ + Ya + 26) dr + | (px S + Pyy + pz) do (4) 
Now when the temperature is constant 
Ovi — 0 Ame gua 5 o o ee (6) 


holds generally as condition of equilibrium. 
Hence we derive from (3), (4), and (5): 


~ /fdw ; Ow Ow Ow Ou Op > 
ty -- Y= = Oe als es WE | Se ed nS Ly 
fe sae Rae Oly Ty 0z- 1 Oy J 022 du, r) 


. 7 » (6) 
= fe (X§ + Yo + 26) dr +f (pis + Pyy + p2S) do \ 


. 


— 


Making use of the relations (2) we get from this after partial 
integration : 


aT We b dw 2 Ow f 
il E — cos (Nie) + a cos (Ny) + - cos (Nz) | + 
7) vy vz 
0 Ou 0 
+ 4 be cos (Na) + a cos (Ny) + = cos (Nz) | + 
+6 an s (Nz) = cos (Ny) + cos (Nz) |. o do — 
ey 0z- 
| Ow ) ’ ) 
\o a Tea eo ee ee 
S iipen: ~ 02x, » Ox, > 0x2) } ° Our (7) 
- (|e) ep ee Te, a 
ie Oa Oy Oz Boe E Ou 
0 ) 1D) dus 5) 
0 * 0 a | \o o ot dlo ay 
zt - OYy ts ME | Lg A 3 Oz, J = 2 Ozy 
Oa Oz ee | Ow a Oy a 
r ost 
ae rae dt =foxs + Yy +Z8)dr +f + pyy + pz$) do | 


The quantities §, 1, and ¢ for the different points of the system 
being quite independent of each other, we obtain from (7) the relations; 


734 


yr — ae ‘0s (Nix) - a) 2 _ Ny pi) 10s (Nz | al 
Px 0 Ves a ( ‘ ) + ary s (i y) + yaa Ss (: 2) == () 
Oxp Ow Ow 
Dy — 0 yoy cos (Na) 4- 2d cos (Ny) + ae cos (| =I) (8) 
: 1Oy» Oy Oyz 
Oy 0 p ow f 
». -- 0 \—— cos (Ne) - — cos (Ny) -- — cos (Nz)) =0 % 
pee |ge em (Ne) + Gr em (NE Gee ON | 0 
Ow a) ow 
uM. Nilaeeat 
: ) (c =) ¢ (¢ in 0 (¢ =| ae 
Sees nee ei 
‘ Ow Ow Oxp 
68) (2) | a 
OY x U Se WEA ae \ . 0 5 ) 
ae On : Oy + Zz are 
dy dy dup 
e Y (3) ; : (e3) ‘ (e5) ee 
ib Sar | iy Oe ae 


If we now introduce the internal tensions Vz, Yy, Ze Y=, Zr, My; 
usual in the theory of elasticity, then hold for the components of 
these tensions on an element of the surface: 

tye ole ee 
¥ v= Y,eos (Nx) -+ Yycos(Ny) + Y= eos(Nz) i .. (10) 
ZN = Z, cos (Nx) + 4, cos(Ny) + Zz (cos (Nz) 
Further in ease of equilibrium : 
pz + Xv=0 pik Yn ==0 2+ Zn =0. 
From (8), (10), and (411) Follower 


ow Ow Ow 
Le = —_ a Wf, — Sie Z: = — 
Pees y Q dy, 2 Oz, | 
F a ‘eae 
Me — Ly = —@ ui Lx = XxX: — ae Xy = Vx ae oo | 
A Oy: 2x ay | 


The relations (12) introduced into (9) now yield the equations 


ya Ok, Oy 0%: 


Ow Oy Oz 

ig Oy Oi. 
—— = -f es 

Ow Oy Oz 
ae 0Z, d0Z, , 024, 


y (13) 


REL re Pale: 


the known conditions of equilibrium for a deformed system, 


735 

2. If we now consider a material element which ean be arbi- 
trarily deformed, we can subject its state to an infinitely small 
variation. With respect to the deformation this. variation. will be 
determined by six mutually independent quantities, three dilatations, 
which determine the change of volume, and three, which determine 
the change of form. Hence speaking thermodynamieally, the Variation 
of state of this element (which need not necessarily be infinitely 
small, provided it is to be considered as homogeneously deformed) 
is determined besides by the temperature, by six mutually independ- 
ent quantities. It now follows from (3) and (12) that for a virtual 


isothermal variation of siaie the following equation will hold for 
the unity of mass 
1 E r r Yr : z oa 
dy = — 33 (Xcae + Vy Yyt Beez + Veyst+ Zpza+Xyty) .. (14) 
U - 


If we now start from the unity of volume, and eall the free 
enerey of it yr, the following form holds for it 
dy! = — (Anez Vy Yy eee Vaya t Duta + Xyity).-, < ~ (15) 
(In this it should be borne in mind. that after the variation the 
volume will in general be no longer equal to unity). 
Now : 
ow 
ue) 
holds generally for the free energy on change of temperature, when 
in the expression for the external work with an infinitely small 
variation no -term with JZ’ occurs as factor. 
Hence: 


STMT e Aiton ie Yaya ete. coe (GU) 


ae 
diy - (Xawx-+ Yyyy+ 2222+ Veyz4+ 2x2 + Xyxy) — dT. (17) 


holds. for virtual variations of state, in which also the temperature 
can undergo a change. 
When we start, from unity..of volame, we have 


dp! = — (Kyte Vy yyjt 4222 is Yeyz+Zyz¢ Xyhy) —7dT. (18) 


where 7 represents. the entropy of the unity. of volume. 


3. Let us now consider a system consisting of two phases, a 
liquid and a solid state. We assume the system to be at rest. Let it 
further as a whole be subjected to the hydrostatic pressure p, while 
arbitrary deformative forces can be active on the surface’ of the 
solid phase, with the exception of that part that is in contact with 
the liquid phase; we exclude volume forces. Consequently the same 

49 

Proceedings Royal Acad. Amsterdam, Vol. XVIL. 


736 


hydrostatic pressure will prevail everywhere in the liquid. We direct 
our attention to a part of the system that contains a portion of the 
boundary plane between the solid and the liquid phase. We assume 
the surface that bounds the considered part of the system, for so 
far as it falls inside the solid phase, to be invariable of position, 
whereas we can subject it to variations of form for so far as it 
falls inside the liquid phase. On this latter part acts then everywhere 
the vertically directed hydrostatic pressure p. We take the part of 
the solid phase that falls inside the considered part of the system, 
as homogeneously deformed. 

Let the considered part of the system contain m, unities of mass 
of the solid phase, m, unities of mass of the liquid phase. The 
direction of the normal to the boundary plane, which points from 
the solid towards the liquid phase, may be called J. 

For the part of the system in question are the free energy, the 
mass, and the volume resp. : 


y=m, p, + m, fp, | 
M=m, + m, \ erreprerme ime ge (1149) 


V = my», + mv, 


when v, and v, represent resp. the volume of the unity of mass 
of the solid and the liquid phase. 

We now subject this part of the system to a virtual change. For 
this purpose we make a small quantity of one phase pass into the 
other at constant temperature. This will be attended with a change 
of the total volume of the considered part of the system. In virtue 
of the suppositions made above this change of volume can only take 
place through the change of position of that part of the surface 
bounding the considered part of the system, which lies in the liquid 
phase. For the rest the state of the liquid phase will not change. 
In order to keep also the solid phase in the same state, to leave 
the quantities determining the deformation unchanged, it will be 
necessary, to make the tensions of the part of the boundary surface 
of the considered part of the system lying inside the solid phase 
undergo intinitesimal variations. Since this part of the boundary 
surface remains unchanged, no work will be required for this. The 
only quantity of external work that we have to take into account, 
will be that which is attended with the change of the part of the 
boundary surface lying inside the liquid phase. 

When dm, and dm, represent the changes of the quantities of the 
two phases, then on account of (19), we shall have: 


737 


dw = yw, dm, -+ w, dm, 
0= dm, + dm, ee ees (0) 
SV =v,dm, + v,dm, 


th connection with the above considerations the work done by 
external forces amounts to: 


dA = — pdbV = — p(v,dm, + v,dm,) . . . . (21) 


If we now apply the condition of equilibrium (5), we obtain, 
making use of (20) and (21), 


Sat Peewee | Daten Pe els ve veh Jone ee (((2id) 
This equation represents the condition of equilibrium for the two 
phases in the case considered here. 


4. Let us now imagine that the system consisting of the two 
phases undergoes a real, infinitesimal change. The condition of 
equilibrium (22) will then retain its validity. It is clear that it will 
give us then a connection between the differentials of the variables. 

As variables determining the state, we choose for the solid phase the 
dilatations and distortions wz, v/y, Zz, yz, 2x, vy, besides the tempera- 
ture 7, for the liquid phase the volume v and the temperature 7. We 
ascribe the value zero to the variables xy, 7, 22, yz, 2x, and 2, in the state 
from which we start (which, however, need not be without tension). 
In order to be able to distinguish the difference between an eventually 
ultimately reached final condition (which need not differ infinitely 
little from the initial condition in mathematical sense) and the initial 
condition from an actually infinitely small change of condition, we 
shall ee the latter by dz,, dyy, dzz, dyz, dzz, day instead of by 
®xy Yys 22) Yxx Fx» Ly, Which we shall use for the final condition that is 
eventually to be reached. This does not alter the fact that the latter’ 
quantities are always treated as if they were infinitely small. 

Proceeding in this way we obtain by differentiation from (22): 


dw, dy, dup, cm Oy, 
dT dity yt — dzz d bs poelle 
or any pele sag. Urayee eg 
(23) 
Ow, Ow, i 
4+ ain ty + pdv, + 0,dp = T OT te es dv, + pdv, + v,dp 


a 
. ia : eH & 
In this ; dx, denotes the increase of the free energy y,, when 
or 
the initial state undergoes a dilatation diz ete., just at this was the 
ease in (3) and the following formulae. 
Now according to the theory of elasticity we have: 


49%* 


738 


1 
(y= ——— (Wa saeiy se Wa) os os 8 ¢ (24) 
Syl 
while further the well known relations: 
Ow, Ow, be 
aT tia eae ne 


hold for the liquid phase. 
On introduction of (12), (24), and (25) we get from (23). 


a ae SEN ats | 
(2],—4,) dT = ip( a >) ar [(Xa—p) dv ++ | 


0. 1 Q, (26) 
Se (Yy —p) dyy IF (2. —p) dzz + Y.dy: =e Zz x aI X dey] 
We can now put: 
r Ll 
Uh = ’ (27) 


T 
-In this we ean call the “heat of melting” 7, by which that quantity 
of heat is to be understood which must be added to convert the 
unity of mass from the solid to the liquid phase, without the con- 
dition of the two phases changing for the rest. We then get: 
abe iy ibe ck Ths 
aT = —|-— —— |} dp + —— [(.— >) dz, --(%—p) aay 
TIO (28) 
+ (4:—p) dzz + VYzdy. + 4,dzz + X,da,| 
When the only deformative force is the hydrostatic pressure, we 
get the known formula of Tuomson and Crausius, since then the 
following equations generally hold: 
Xx — p=0 iy —p=0 Z.—p=0 | 


N2 Sy 


29 
Y.=0 Z,—=0 x Oe ee) 
Tefal 1 
dT = — (= ~ da ere (3X0) 
7 \Os 01 
If on the other hand dp = 0, we get: 
dT = —— [(X.—p) dre + (Yy—p) dy + (Zp) dee + | 
Pre Or (31) 
+ Y.dy. + Z,dz, + X,dxy| | 


Since the form between square brackets, provided with the negative 
sign, represents the work performed in the deformative forces, with 
the exception of the pressure p, a deformation will bring about a 
lowering of the freezing point, when this work is positive. 


5. We shall now assume that the initial state (for which we put 
Vay Yyy Zz Yzs 22, ty. EQual to zero) is to be considered as without 


739 


tension. In this case (81) will also be applicable; we may then, 
however, replace 7 and e, by 7, and o9,,, in which 7, denotes the 
heat of melting, and o0,, the density of the solid phase in the tension- 


less state; then we have 


Tt 
dT = —— [(Xs—p) dts + (Yy—p) dyy + (Z—p) de. +| 


PP 10 


ro 
+ Y.dyz + Zdzz + X,day] 

If we disregard quantities of the second order, which we are 
allowed to do when we consider the dilatations and distortions 
as infinitely small, we can integrate (32), placing 7, r,, and @,, 
outside the integral sign. We then get for the lowering of the freezing 
point in the state determined by @z, Wy. Zz, Yes Za Vy, 


vy 


T 
PQ r0 


Uz «ae 
f (eo ie ae eae 


AL = 
0 


(33) 


Y.dyz =F Z,dzz + X,da| 


The heat of melting in the state determined by 2,, yy, 2:. Ys, Zr, dy 
will differ- from that in the tensionless state by an amount that is 
of the same order as the dilatations and distortions themselves. For 
an infinitely small change follows for the change of the free energy 
from (14): 


1 
dy = — — (Xzdxx + Yydyy + Z.dzz + Y.dyz + Zydzz + X,day) 
o 7 : 


Hence the difference in free energy between the deformative and 
the tensionless state amounts to: 


HAS exo IES Do 


all 
sh = =! — [Xzdxy 4+ Yydyy + Zdzz + V.dyz + Zrdzz + X,da,]. 
0 ye, 
0 


For the difference in entropy between these states follows then 
from (16) 


y 


Te ceo Pick 
0 28 
Ay = at [Xzdaz + Vydy, + Z.dzz + Yzdy: + Zrdzez + X,de,]. 
(sae 


From (27) follows then for the difference in heat of melting: 


ditty Cis Eno 
6) fll 
Ar = — T— {= [Xida,z-++ VY dy,4 Zdzz+ Y.dyz+ Zyde,+ Xydx,| (34) 
or Q k : 
0 


740 


This will also apply to the case that the initial state is not 
tensionless; only (384) does not represent then the difference in 


melting heat between the state v,...yz... and the tensionless state, 
but the difference between the state a,...y:z... and the initial state, 


which is not tensionless in this case. 


6. Let us now suppose that forees act on the surface of the 
solid phase which are exerted by solid bodies which rest on the 
solid phase, and in consequence of the presence of which the sur- 
face of the phase is not in contact with the liquid phase. We can 
then imagine that a small part of the solid phase that is in contact 
with the solid bodies which exert forces, is converted to the liquid 
state, without the solid bodies changing their places. For this case 
we can again draw up the condition of equilibrium. 

We take the boundary plane of the solid phase as X Y-plane, and 
suppose that the Z-axis is the normal to this plane which is directed 
from the solid to the liquid phase. For the total free energy, the 
mass, and the volume the following relations hold in this case: 


Y—m, yp, +m, wp, 
M=m, +m, Mier. tc. « (23); 
V=m,v, + m, », 


Let now an infinitely small quantity of the solid phase be con- 
verted to the liquid phase, then: 
JE = mdw, + w,dm, + mdi, + ,dm, . . . (36) 
During the conversion the volumes v, and v, will have to change, 
as the total volume remains constant, as we supposed. The considered 
change being a virtual change, we may assume that as far as the 
solid phase is concerned, this change is brought about by variation 
of z- alone. Then we get: 


Ow, 

OU —— 20220 3 os 9 5) 
Further : 

ge Ou, ; ae 

Cae carrag Nes SCCM IEON IO 5 1 ici « ((ic\) 

By introduction of (87) and (88) into (86) we get: 

he Op, dw, 

OF =m, au diz 3M; Fatt dv, + dm, + w,dm, . . (39) 


Just as before (see above under 3) the tensions at the surface that 
bounds tne considered part of the system will have to vary now 
too. We supposed, however, that this surface does not change its 


741 


position, so that no work will be done by external forces. The 
condition of equilibrium is now: 


Oui Qe eters tae e.g | (A) 


We must use here the double sign seeing that there is only a 
conversion possible in one direction. The sign = will hold for the 
boundary equilibrium, i.e. the equilibrium at which a transition from 
the solid to the liquid phase will just be possible. Now the equations 
(35) give further ve 

dm, + dm, = 0 


: 41 
m, dv, + v,dm, + m,dv, + v,dm, = 0 ( y 
in addition we have 
1 
OSS = Uae on 0 ro (IBF 
Qe; An : 


If we limit ourselves to the boundary equilibrium we get from 

(12), (85). (89), (40), (41) and (42) making use of the equation 
Z, — p= 0*. i faliQet os? Soi 
Wit Pepe tpl, «= = |S 5 lee) 

Hence we get the same relation as condition of equilibrium between 
solid and liquid phase as we had for the case that the two phases 
were in contact. Therefore the conclusions about the lowering of 
the freezing point will also be the same. Of course as pressure on 
the solid phase must then be taken into account the hydrostatic 
pressure, to which must be added that which is exerted by the 
solid bodies which are on the solid phase. 

7. We shall now consider more closely the amount of the lowering 
of the freezing point, in which we shall make use of the expres- 
sion (32). To caleulate this amount it is necessary to know the 
relation between the quantities x... y:...andthe tensions X,... Y.... 
In the most general case, the quantities 2... y:... being considered 
as infinitely small quantities, we shall be allowed to assume a 
linear relation of the form: 


Xx S Oy, @e + Oy gYy F Oy ,%z FO Yo Ah Gyytz + yy ity 


: me ae a : : (45) 
Ve yy + Oy yy + Gy,22 + Oy Ye FOyee Qo hy 
in which 
Pia Ge fe Ss ee (AG) 
will generally hold, because the tensions X,... ¥.... according to 


(8) may be considered as the partial differential quotients of the free 


742 


energy per unity of volume taken with the negative sign. Further 
the coeflicients «@ must be considered as functions of the temperature. 
To this most general case, in which the number of coetficients amounts 
io 21, answers a crystal of the lowest symmetry. This leads, of course, 
to very intricate calculations. ‘ 

We prefer, therefore, to consider the simplest case, viz. an isotropous 
body. For this holds, if we use the prevalent notation ’). 


 — ale lee is BX (vx a Yy + z 2) (47) 
Seas ae ity, : 
from which equations can be derived ; 
sear six z gr YA 
ot Se eke ae Sa C2 + y »|| 
Y,=— —YV, 
K 
In this the relation : 
136; 
a es 
“7420 ae 


exists between the coefticients AK and @ on one side and the elasticity 
coefficient / on the other side. - 

Let us now consider a circular cylinder, the axis of which coin- 
cides with the Z-axis. Let one end be rigidly fastened, while forees 
resp. couples act on the other. Let the length in the direction of 
the Z-axis be /, and the radius of the cylinder &. The conditions 
of this problem may be satisfied by putting oo 

Xp == xy == () Y,—=09 merely seni, 11,1 (240)! 

If P,, Py, P; ave the components of the force, Qe, Q,, Q, the com- 
ponents of the couple acting on the end plane, then for the other 
tensions hold the expressions : 


jen Mer Walsr aie hayes AP oe ease eave 
Tips = a | © 1 2 Sere han, 
ner wee hie ae aa Sa = 

3s sy * PP. 86) (R2—2x)—y? - P, 1446 
5 Px (8 +89) ( eee ay EM 

aR* | 2k 1436 Ri1430° 
age 2Q..%@ b, 1446 P, (8+ 84) ( (R?—y* ice =i 
“" @R! 2R1+30 oa peat 538 
Further : 


_ 3) Cf. among others G, Kircurorr, Vorlesungen tiber Mechanik, 


143 
ip 0 ape ea ez - 
126 
E1260 
See Ie re (52) 
21430 
E1+26 
Fico eile Ys 


We shall now discuss some special cases. 
1. Compression resp. extension. 
In this only P:=£0 is put, from which follows : 
La Pe Ne SS) 
aR? 
(in this the liquid pressure p is neglected). 
Then the lowering of the freezing point is 


it 
AT =— [ete 
7,0 


oso 


Making use of (52) and carrying out the integration, we get : 
tee 


si OF 
7.0, 2h 


AT = — 


which formula is in perfect concordance with Rinckw’s. *) 

We apply this to ice, which we shall treat as an isotropous 
substance. 

RieckE assumes 0,7 ke. for the drawing-solidity of ice per mm’, and 
calculates with this O°.017 for AT. As for most substances the 
_pressing-solidity is considerably greater than the drawing-solidity, this 
diminution can probably be made larger in the case of compression, 
so that it can be measured comparatively easily and with suitable 
apparatus even the just mentioned lowering of the freezing point 
would also be liable to be measured. 

2. Sagging. 

In this case we only assume that P,==0. When we consider a 
point for which «= Rk, y = 0, then it follows from the formulae that : 


Py 1420 


i) =) Ve é 
ah? 1+-30 


The lowering of the freezing point of the considered point is: 


1) E. Rirexeg, loc. cit. p. 7386 form. (20), 


744 
Making use of (52) we get after integration : 


T +30 Y# 
TRo, 15208 Sa 


(i 


In order to obtain a limiting value for Y., we make use of the 
results of an investigation by Hess’) on. the sagging of ice 
erystals. He charged a crystal 2.9 em long, 1.0 em broad, and 1,2 em 
thick at its end with a weight of 5000 grams, without rupture taking 
place. Let us assume by approximation that an ice cylinder of a 
diameter of 1 em could bear the same load. We can then derive a 
limiting value of VY. from (54). 

If we introduce this into (52), we find finally, assuming that 0 = 3, 
which is about correct for a great many substances, — 1.19 x 10-4 — 
degree for AZ, which quantity is probably not lable to measure- 
ment. That this quantity is so small, is the consequence of the sinall 
value of the maximum tangential tensions which ice can bear. 

We considered the point on the circumference for which «= R, 
y=0. If on the other hand we take the point for which w= 0, 
y= Rk, we get the formulae 


4l 


Yin = 
ak? 


Py Mos Wa =O, 


If as before, we again assume that an ice cylinder of a diameter 
of 1 em. can bear a load of 5000 grams at its end, we find for Z, 
a value which appears to be greater than the value assumed ‘by 
Riecke. If we calculate the lowering of the freezing point by means , 
of this, we find 4 7’—= — 0°.081, an amount that can be easily measured. 

We see at the same time that the lowering of the freezing point 
has different values at different points of the surface; a state of 
equilibrium is therefore impossible. The rod of ice will diminish on 
the upper surface and on the lower surface, and that much more 
quickly than on the sides, which will also diminish a little. Further 
this diminution will increase towards the end where the rod is loaded. 

3. Torsion. 

In this case only Q-—|—0. From the formulae (51) follows then 
for the point 2=0, y= & 


2Q. 


Viet) x, = — 3 
aR 


Taking the small amount of the tangential tensions which ice can 


1) H. Hess Ann. d. Phys. 8 p. 405, 1902, 


745 


bear into consideration, the lowering of the freezing point will again 
become very small in this case. Since the tangential tension all along 
the cylinder surface has the same value, equilibrium with the sur- 
rounding liquid will now be possible. 


Haarlem, May 1914 Physical Laboratory of 
“Tryier’s Stichting’. 


Physics. — “The effect of magnetisation of the electrodes on the 
electromotive force.’ By Dr, G. J. Er1as. (Communicated by 
Prof. H. A. Lorentz). 


(Communicated in the meeting of June 27, 1914). 

1. The question in how far magnetisation of the electrodes is of 
influence on the electromotive force in a circuit in which there are 
electrolytes, has already often been examined, without it being 
possible to derive a definite answer to this question from the results 
of these researches. Thus Gross') found no definite direction of the 
current in concentrated solutions of ferro salts, while in concentrated 
solutions of ferri salts the magnetized electrode (both electrodes 
consisted of iron) became the anode. ANDREWS”) arrived at the same 
result working with strong acids as electrolytes. NicHois and FRANKLIN *) 
obtained results which were in concordance with those of Gross 
and ANbDREWs, in case a pole of a magnetized iron rod came in 
contact with the electrolyte, which consisted of a solution of chromic 
acid. In this case the electromotive force greatly increased with the 
magnetisation, and reached the value of about 68 millivolts in a 
field of 20000 Gauss. If on the other hand the neutral region of 
the magnetized rod was in contact with the electrolyte, the sense of 
the electromotive force was opposite. Row1nanp and Bru‘) found 
that the magnetized electrode became cathode when acids that 
attacked the iron, were used as electrolytes. Squirr*), who took 
nitric acid as electrolyte, came to the same result. The maximum 
electromotive force amounted to 36 millivolts, in a field of 10000 


1) Tu. Gross. Sitz. Ber. d. kais. Ak. d. Wiss. 92. Dec. 1885. 

2) ANDREWS. Proc. Roy. Soc. 42 p. 459, 1887; 44 p. 152, 1888. 

8) E. L. Nicpots and W. 8. Franxur, Am. Journ. of Science 31 p. 272. 1886; 
34 p. 419, 1887; 35 p. 290, 1888. 

4) H. A. Rownanp and L. Bextu. Am, Journ. of Science. 86 p. 39, 1888. 

5) G. O. Squmer. Am. Journ. of Science. 45 p. 443, 1893, 


746 


Gauss; on further strengthening of the field this amount did not 
change. Also Hurmucrsct *) found the electromotive force in the same 
-sense, when diluted acetic acid or oxalic acid was used as electro- 
lyte. In a field of 7300 Gauss the electromotive force amounted to 
14 millivolts. Finally Bucanrer*) has occupied himself with this 
question. His result is in so far entirely negative that he finds no 
electromotive force which would reach the value of 10~-° Volts for 
neutral solutions of ferro salts in the case of magnetisation of the 
electrode in a field of 1200 Gauss. He further pronounces the opinion 
that the electromotive forces found by Rownanp are caused by 
mechanical disturbances of the equilibrium (‘‘Erschiitterungen’’), which 
would be the consequence of the origin of the magnetic field. Then 
Bucuerrr compares Hurmucescu’s results with what has been theoreti- 
cally derived by Dunem*), and coneludes that no concordance exists 
between them. Dune arrives at the formula: 


/ERY 7 i 
ad .% (1) 


in which / represents the magnetisation of the electrode, 2 the electro- 
chemical equivalent of the iron, x the susceptibility, and d@ the 
density, the electromotive force / being taken positive, when the 
magnetized electrode is cathode. When we eliminate H;, /, and # by 
the aid of the relations: 

B= H;+ 421 33 he Jal Th03 5156 


we get instead of (1) 
R ioe Al i S| (2 
t= Gada hi co, 


It has appeared to me that in consequence of an inaccurate expres- 
sion for the energy of a magnetic field, this value of / is about fe 
times too small, so that we may write by approximation because 
has a large value: 

f IB oh: 
P=. 


which expression, however, only holds when the electrolyte is a 
neutral iron solution. 
When the experiment is arranged in such a way that 5 may be 
put equal to the external intensity of the field H7, we see from (3) 
1) Hurmucescu. Eclair. Electr. Nr. 6 and 7, 1895. 
2) A. H. Bucnerer. Wied. Ann. 58 p. 564, 1896 ; 59 p. 735, 1896 ; 61 p. 807, 1897. 
5) P. Duuem. Ann. de la Fac. des Sciences de Toulouse, 1888—89. Wied. Ann, 
Beibl. 13 p. 101, 1889. 


; 747 


that the electromotive force would have to increase with the square 
of the intensity of the field. On introduction of the values for iron 


7 == 29 So INS Gees d=7.9 
we get for 
H = 10000 Gauss ESOS = 2 Wot 


In Bucnerer’s experiment the intensity of the field was 1200, if 
the induction 4 bad had the same value, the electromotive force would 
have been 2.4 x 10—* Volts. As this amount is much less than the 
smallest value whieh Bocnerer could measure (10~° Volts), its negative 
result cannet be considered in conflict with the theoretical resuit. 

The results of the other investigators, who worked with acids as 
electrolytes, ave not at all in agreement with formula (3), in fact 
they could hardly be so, as (8) rests on the supposition of a neutral 
iron solution. 

As the case that the electroiyte is a dilute solution of the metal 
of electrodes, which is assumed to be equal for the two electrodes, 
is the only one that is liable to exact thermodynamic treatment, | 
have calculated the value of the potential difference for this case in 
what follows. Further I have communicated the results of experiments 
made on this subject. 

2. Let us now consider‘) an arbitrary system in which also 
electric currents and magnetic fields can be present. As variables in 
this system we choose the temperature 7, further a number of 
geometrical quantities «,,«@,..., and finally the magnetic induction %; 
when the last quantity is known everywhere, then, besides the 
magnetic field. the electrical current is also determined everywhere. 
The external forces exerted by the system, are the components of 
force A,, A,... corresponding to the geometrical quantities, besides 
the external electromotive forces &,. In order to be justified in leaving 
JouLr’s heat out of consideration we shall assume that the conductors, 
for so far as a current passes through them, possess no resistance. 
We shall further assume that the system loses no energy by electro- 
motive radiation and we exclude currents of displacement. 

If the .system undergoes an infinitely small virtual variation, we 
first inquire into the work performed by the system on its surround- 
ings. If .the variations of the geometrical quantifies are d« 
the corresponding work can be expressed by 


ny Olersa op 


1) The train of reasoning on which the general method of treatment followed 
here is based, was suggested to me by Prof. Dr. H. A. Lorenvz, for which | will 
express here my heartfelt thanks. 


748 


a A da, Apdo Dom tiete G Oe 


Further the external electromotive forces will perform work per 
unity of time equal to 


dW, Ca 
——— = | (©, €) .dr 
dt 


in which © denotes the electrical current. The work done by the 
system amounts, therefore, per unity of time to: 

dW, 
=—{(€.§), dr. 


For this we may write: 
dW, 
— fe + €,, @) dr +{G €) dr, 


in which € denotes the electrical force. Now in the conductors 
¢ — o(€ +- &,). 
From the supposition that in the conductors 6 will be infinitely 


large, follows that here € + €, must be = 0, whereas outside the 


x : F dw* 
conductors © =0. Hence the first term in the expression for 


disappears. When we make use of the expression : 
$ =ccurl f°) 


we get after partial integration 


dW, 
r= fe curl ©). dr4- oft. ely. de. 


The second term disappears on account of the supposition that 
no energy leaves the system through radiation. We finally get then 
by the aid of the relation: 


Pagers ee 


Ot 


dW. 0d 
= — Jagp——= lo @ 
at, wah re a Ot ) a 


If the variation of 8 in the time dt is JB, we get: 


BW, = — {(9, 4%). dr, wt. ae 


The total work performed by the system now amounts to the 
sum of (4) and (5), 


1) Here Lorentz's system of unities is used. 
y 


749 


SW = Ada, + A,da,4+ .. —[o 1 GR5))in Che oF oo (3) 


If we now introduce the free energy of the system, the following 
well known relation holds for it 
w= E—-T.H 
when E represents the internal energy, H the entropy. For au 
infinitely small variaton we get from this: 
JW = dE—T . dSH—H. dT. 
Further 
T.dH= dQ=dE + dW, 


in which dQ is the quantity of heat added to the system. Making 
use of (6) we get from this: 


dW — Ada, —A,da,.... + [ (9,08) de— a 


Let in a certain initial state, in which the variables a,,a,.. 
have the values «,,, @,,-- 
energy ¥,. In the magnetic state, in which & will have a certain 
value everywhere, and the temperature and another quantity, e.g. 
the external pressure have remained constant, the geometrical 
variables will assume other values, which we shall denote by a,, @, .. 
We can now make this transition take place in two steps. We first 
give the geometrical variables the values «,,a,, 8 remaining = 0; 
hence the free energy will increase by an amount A, W% 

Further, while a,,@,... remains unchanged, we can bring the 
magnetic induction B from zero to the final value; then the free 
energy will inerease by Ay. In this way the final state is reached, 
in which the free energy will be: ; 


v= UW+ A w+ Aut . . . . ’ . (8) 
Then according to (7) the following equation will hold: 


by t= f [19 AB) de 5 3 SG oe ee (M)] 


3. Let us now return to the above discussed case, in which two 
electrodes of the same metal are placed in the dilute solution of a 
salt of this metal. The concentration of the solution can be different 
at different places. We think the circuit closed by means of a wire 
connecting the two electrodes. Let one electrode be in a magnetic 
field, in consequence of which it is magnetized. We think the 
magnetic field excited by an electromagnet, the leads of which 
possess no resistance, 


.. © being = 0, the system have the free 


750: 


In the second eireuit in which the electrolyte is found, we think 
inserted an electromotive force -— /, which is in equilibrium with 
the electromotive force /’ existing eventually in consequence of the 
presence of the magnetic field; we shall assume that sense of circuit 
which is directed inside the electrolyte towards the magnetised 
electrode, to be positive. We shall assume also the resistance of this 
second circuit to be zero. 

We shall subject this whole system to an infinitesimal variation. 
Let this variation consist’ in the passage of an infinitely small 
quantity of electricity e through the second circuit, and that in that 
sense that is directed inside the electrolyte towards the magnetized 
electrode. We shall moreover ‘assume that in this variation the 
magnetic induction remains unchanged. in all the points of the’ 
system. We shall further assume that the surface that bounds the 
second circuit, does not change its position. 

In the first place we shall consider the work of the external 
forces. These forces consist of: 1. the electromotive forces in the 
first cireuit (that of the electromagnet); 2. the electromotive force 
— FF in the second circuit; 3. the external pressure p. As we have 
supposed % to remain constant in all the points of the system, the 


[dwt 


Which represents the flux of B through the first cireuit will not 
change either. It follows from this that no electromotive force is. 
active in this circuit, so that the work of this force is zero, The, 
electromotive foree —# in the second cirenit will perform. work. 
equal to —.e, when a quantity of electricity e passes. The whole 
volume of the second circuit being supposed constant, the work of 
the external pressure will amount to zero. 


value of 


In all the work performed by the system is therefore 
OW = Ee. ss 


Let us then consider the change of the free energy of the system. 
For this purpose we shall examine what are the consequences of 
the passage of the quantity of electricity e through the electrolyte 
in the direction of the non-magnetized electrode towards the mag- 
netized one. We shall eall the former the anode, the latter the 
cathode. 7 

If w and v represent the absolute values of the velocities of cation. 


751 


and anion in the solution, then n= is the quantity which 
v 
Hirrorr has called “Ueberfiihrungszahl” of the cation. 

Of a current i the part n.t is carried by the cation, the part 
(1—n).i by the anion. So the number of gram equivalents of the 
cation in the unity of volume will increase per unity of time by : 

L is 
. ee ec) = aay 

as div.i—0 is; represents the charge of a univalent gram ion. 
In the same way the number of gram equivalents of the anion will 
increase by the same amount per unity of time, so that the solution 
will remain neutral. If / is the valency of the molecule, and m the 
molecular weight, the mass of the salt will increase per unity of 
time by an amount: 

GO 5, 

= (i, 7). 

If the quantity of electricity e, passes through the unity of surface, 
and if i, represents the unity vector in the direction t, the increment is: 


m.eé 


dy = —— (I,, yn) - Sh cies, ives bas) Migs (GL) 
k.g 


In the volume elements which lie on the surface, the increment 
of the mass of salt will be per unity of surface : 


Re eo gee tk ke AN 


when NV is the direction of the normal directed inward. The total 
quantity of salt inside the solution will now increase by an amount: 


fo + fara] fo Cooma + fet. nda] =o 
S ease) 8 


7 
When we apply Gauss’s theorem and make use of the equation 
divi = 0. The quantity of salt, therefore, does not change. 

The only change consists in this that the concentration in the 
different volume elements is modified, and that a quantity of elec- 
tricity e dissolved at the anode, has deposited at the cathode. 

We shall examine what change the total free energy of the 
system has undergone in consequence of what has taken place in 
the electrolyte. Above we found the expression (8) for the free 
energy, (9) holding for the “magnetic”? part of it. We further chose 
the variation so that the magnetic induction did not undergo any 
change. In the first place we must now take into account that at 

50 

Proceedings Royal Acad Amsterdam. Vol. XVII. 


(52 


the anode a certain volume of iron has been replaced by the solution, 
whereas at the eathode the solution has been replaced by iron. The 
Gy . . 
volume of iron —.—.— will correspond to the quantity of elee- 
( Fy 3 
tricity e, when a denotes the atomic weight, 4, the valeney of the 
atom, « the density of the iron. If we assume that at the anode 
no magnetic field is present, the substitution of iron solution for 
iron will not bring about any modification in the magnetic part of 
the free energy. At the cathode, however, this substitution will give 
rise to a change in the expression (9), which, when «, represents 
the permeability of the iron solution, uw that of the iron, amounts to: 


b b 
! a.e ES 183 
Jd (AyweY)= a he ee ea Bi ae cee . . (13) 
0 


when B means the absolute value of 3 and B this value at the 
- eathode. When we speak of “at the cathode” or “at the anode”, 
we mean by this that we must take the value of the considered 
quantity at a plane that is at a very small distance from the 
cathode resp. anode, this to evade the difficulties which the phe- 
nomena taking place in the boundary layer might cause; we 
shall examine this question more closely further on. On account of 
the smallness of the considered volume we may assume that the 
value of £B is the same everywhere inside the volume. If we put 
u, = 1+ 4x,, in which «,, the susceptibility per unity of volume, 
is to be considered as a small quantity, we get about : 


B 


> 


x a.é B _ B 
d(AyW)=— |= (1 dare, — [58 aes 
0 


when x 


0 


represents the susceptibility at the cathode. If we assume 


1 
u to be very great for iron, so that — is to be neglected with respect 
Uu 
to unity, and if we replace B by H, the absolute value of the inten- 
sity of the tield in air at the cathode, we get: 


6 (4uY)=—s7— — (1—Az'x,) (2 1 eee 
Instead of (13), using the relation : 


1 
B(1——)=4e4, 
u 


in which / is the absolute value of the magnetisation we may 
further write : 


753 


B 

Age ath ee = 
J, (Au ¥)= - ———.]fCU—T,)dB. . . . . (16) 

Dak neon 

0 
We must further take the changes of concentration in the different 
elements of the electrolyte into account. If we introduce the concen- 
tration ¢ as the number of grammolecules of the dissolved substance 
per unity of mass of the solution, this is modified by the passage of 
the quantity of electricity e. If the density of the electrolyte is @, 
then the variation of density, when the volume remains unchanged, 

will amount to: 


QOS U0 6 6 56 0 neyo A(hM)) 


in which dy is given by (11) and (12). By means of this we find 
easily for the change of concentration : 


1—me 
Jc = 0p Set i ee ee oe 8, (LS) 
mm. 0) 
Now for dilute solutions very nearly : 
YR Ole Cee Wien ail gts reassess (LO) 


holds, in which x is the so-called absolute specific susceptibility per 
unity of volume; which is considered as independent of @*). We 
get from this by the aid of (17) and (18): 


Ota ODr. 
This then gives, as x, must be considered as small : 
B 
| f) dB = — 2a By dv. 


0 
When we multiply this expression by the volume element dr, theti 
introduce the value of dy from (11) and (12), and integrate witli 
respect to the whole volume of the solution, we get: 


f 2ay.m ‘ PITTA TIN {ise 
J, (AuW) = — - TA (Be liu gn) = | [ae och iy t do. 
V Ss 
If we assume n to be constant, which is permissible, on account 
of the relative smallness of this term, if we suppose further that 
at the anode B=O, at the cathode in air B=—H, we get: 


2TmM.y.en — 


J, (Au ¥)= Taree! Alo Hee oe (20) 


1) Relation (19) holds of course only as long as the specific magnetic properties 
are independent of the concentration. 


50" 


~I 
ox 
rss 


as for the cathode holds : 


— forty dome. 


4. We must further consider the change of the “non-magnetic” 
part of the free energy; as we saw above the values must be 
assigned to the variables which they will have in the magnetic field. 

The only change which is involved in this, is the change of con- 
centration of the solution. If the free energy of the unity of mass 
of this is w, then that of the volume of solution @ of density @ is 

d¥Y, =0.o0.e, 
when ¥*, is the free energy of the solution. When we make use of 
(17) and (18), and further of the relation : 


ow 
=== — oe eee (te 
ae P (21) 
which follows from (7), the variation of this will amount to: 
: 7 Ow 1—me 
dd, = dv ly + P + =| BD 5 (2:2) 
Q 0c m 


For the free energy of the unity of mass of the solution we shall 

use the well-known equation : 
w=w, tact per+... .+ RVelogc,. . . . (28) 
in which yw, means the free energy for c= 0. 

In this we must give to the variables c and v the values which 
they possess in the magnetic field in the state of equilibrium. 

On the other hand we can, however, also imagine that different 
concentrations can permanently exist in the different volume elements 
of the solution, in such a way that no change can be brought about 
in this by the magnetic field. Thus we shall obtain the potential 
difference between the electrodes on arbitrary distribution of the 
concentration. The supposition made is a fiction; the more so as 
we have assumed also the resistance equal to zero; in general the 
velocity of diffusion will namely increase as the resistance decreases, 
with which permanent concentration differences are in contradiction. 
This supposition, however, must always be made for such problems, 
in order to be able to apply the laws of the reversible processes ; 
hence we also make them here. 

With the aid of (22) we get from (21) 


E p RI a 
dd ¥, = dv | w, +— + — (1 + loge) — RTc + — | .w. 
0 m m 


When we use here the expressions (11) and (12), and integrate 


755 


over the whole volume of the solution, we get: 


7 


m : RI 
Cie = fe . (i, ’ vn) : EB — =. == (1 ai log oj hie ar =| . at 
m m 


kg . 


m jo. aya Fa a 
+ = | é.in,.2.| wp, +— + —(1 + loge) — RTc-+ —1|.do. 
hg 0 m m 
& a 
When we take n again as constant, we get: 
mM. e@ 1 1 Iiedhe 
a — =.—1%, —wW,, t$pl— — — | + —log—— RT (c,— of 
k Eas OE, Qs, ue C5 = 


when we denote the quantities referring to the anode by the index 


1, those referring to the cathode by the index 2. 
We may further write: 


bos = Won + (2) 


or, because 


OW, 
jiiwase 


1 1 
Woo =U. + P{ ———}- 
Q, 02 


There remains finally 


mn 


1 : 
US ret Rt | To? =e —0)| | joy cue (24) 


e 
Ԥ m Cy 
From the well known theorem for the free energy : 
dv 4+ 6¢w—0 
we get with the aid of (10), (16), (20), and (24): 


B \ 
pee. PO ot) | 
ji — (1—T,) dB — - oaks 
d kg 
0 


Ww a. 1 C 
-— . RT .| —log — — (¢,—e,) 
kg E Os | 

in which 4 is the electrochemical equivalent of iron. 

Hence the potential difference consists of two parts, viz. oue part 
(the first two terms), which depends on ‘the magnetic field, and a 
second part, which depends on the concentrations at the electrodes. 
The second term of the first part will increase proportional to the 
second power of the external intensity of the field, the first term, 
too, in case of small intensities of the field, where we may replace 
(16) by (15); at great intensities of the field, however, / will reach 


756 


the value of saturation, so that this term — which far exceeds the 
other “magnetie’? term — will increase only about linearly with 
the external intensity of the field. The sense of the electromotive 
force determined by the first term is directed inside the solution 
from the non-magnetized towards the magnetized electrode. The 
second part of the expression becomes equal to zero for c, =e, ; 
with neglect of the contraction which the solution undergoes on 
concentration, this expression agrees with the potential difference - 
calculated by Hertmno1tz'), between two electrodes which are in 
solutions of different concentrations. 

If we assume c,—c,, and neglect the terms which depend on 
the suseeptibility of the solution, the following form holds for not 
foo great intensities of the field (in which « is still to be considered 
as very great) i 


phe (26) 
2d 
If we use electromagnetic unities, this becomes: 
SF aah 
7 Smad’ 


which agrees with (38). 

In order to simplify our considerations we have disregarded the 
transition layers between iron and electrolyte; in them phenomena 
will namely take place which cannot be examined in detail. It now 
remains to prove that in the caleulation of the free energy the in- 
fluence of these transition layers may be neglected. For this purpose 
it is necessary to assume that the thickness of the transition layers 
is of the order of magnitude 7, when / represents so small a quantity 
that we may assume that inside the thickness / the liquid is in 
equilibrium with the electrode. We shall further assume the limits 
of these transition layers on one side inside the iron, on the other 
side inside the solution. Let the quantity of electricity e, which we 
have passed through the solution, be of the order of magnitude §; the 
same thing will be the case with the thickness of the iron layer, 
which has dissolved at the anode, deposited at the cathode. This 
iron layer may be infinitely thin with respect to the thickness of the 
transition layer, and entirely fall within it- 

We have already taken into account the change of the “magnetic 
part” of the freé energy, which is the consequence of the displacement 
of the iron and the dissolved substance. Now we have still to take 
into account the change of the state of the transition layers, which 


1) H. Hetmunoirz. Wied. Ann. 3 p. 201, 1878, 


Miel 
TOM 


is the consequence of the conveyance of iron and dissolved substance. 
The quantity of dissolved substance supplied resp. extracted in the 
transition layers is of the order £, just as the quantity of electricity 
e. As the volume of the transition layers is of the order of magnitude 


/, the change of state inside these layer will be of the order 7 


Now there was equilibrium in the transition layers before the 
variation; hence a variation of the free energy per unity of mass 


2 
of the order of magnitude (=) will correspond to a change of state 


§ ; ae 
of the order 5 (the external work is zero). The variation of the 


total free energy of the transition layers will therefore be of the 


Yeo 


s am 
order qe Thence we see that this variation may be neglected with 


respect to the other variations of the free energy, which are of the order §. 


5. We shall now still examine what will be the equilibrium 
concentration in the magnetic field, i. e. that concentration which 
will finally exist after the diffusion has been active between the 
different volume elements. For this purpose we consider an infini- 
tesimal variation of the total free energy YW of the system. We 
choose this so that all the parts of the system, with the exception 
of the solution, remain unvaried ; moreover we leave the magnetic 
induction 3 unvaried. We can, therefore, restrict ourselves to the 
variation of ¥Y, the free energy of the solution in the magnetic 
state. For this free energy holds the expression according to (8) 


and (9): 
Ue = || le w+ | 13) 25 |r, 


when we use the expression (23) for w. 
As the susceptibility may be considered as small, we may put 
Ore ail € 


a Jew 4G O—daay) [ae co 5 of 6 (8H) 


We shall now let the variation consist in a change of the con- 
centration, accompanied with a change of the specifie volume ; in 
this we leave the volume of every volume element unvaried, so 
that the external work is equal to zero. We get the relation between 
concentration variation and volume variation by eliminating dg from 
(17) and (18), by which we get: 


6c = 10 fo a ee eed 


mo 


Now we get from (27), keeping in view that 6 remains unchanged: 
Je, = fle .dy+w . do —20 B* dx, | dr. 
Making use of (19), (21), and (28) we get from this, when we 
apply the thesis of the free energy : 


OI; 1—mc 0 
[ [e+ e+ Pane y|.0e.dr =o 
Sie de 


@ m 


Further exists the relation : 


fe seh SUE 


the total mass, from which follows : 


[a Ton 0: 


— 0 
s ue w+ Tactics ~ —2nxB* .y¥ = const. . .’ ee) 
c 


me 


The formula 


follows from i two relations as condition of equilibrium for the 
solution in the magnetic field. For this we may put, just as above 
in the expressions (22) 
P RI a a “ 
hy + — + —— (1 + logo) — RT¢ + — — 2B. = const, 


m m 


ry 


from whieh follows, because at the anode B =0, at the cathode B=A, 
just as above for (24): 

RT ; 

— log? — RT (c,—c,) = 2ay. 7). . « + G0) 


Mm Cy 


K 


5), we get for the potential differ- 
ence in the state of equilibrium, at which also the solution is in 
equilibrium 


When we introduce this into (2 


B 
Ae 
= (I=1) dB.) 2 ne 
€ 


0 


6. In order to test the obtained result by observation, IT madea 
number of experiments, in the first place with iron. The iron 
used for this was electrolytic iron, which Prof. Franz Fiscumr at 


1) With ee of the contraction which the solution undergoes, this result is 
in accordance with the result derived by Vorar (Gétt, Nachr. Math. phys. KI, 
1910 p. 545), 


759 


Charlottenburg kindly procured me. The magnetized electrode con- 
sisted of a circular plate, which was of the same size as the pole 
plane of the electromagnet, and was rigidly fastened to it, a glass 
plate serving as isolation. The other electrode was outside the field. 
The concentration of the used solution of ferrosulphate was generally 
5°/,. The results obtained with this may be summarized as follows. 
On excitation of the magnetic field I always obtained a current in 
the sense as the theory requires. The extent of the obtained effect 
differed, however, greatly from the theoretical value ; the measured 
potential differences were, namely, between the strengths of the 
field O and about 20.000 Gauss 10 or 20 times as great as the for- 
mula would require. At first the course was about proportional to 
the second power of the strength of the field, the effect reaching a 
value of 6.38 « 10-4 Volts at about 16000 Gauss, which did not 
change on further strengthening of the field. If the used solutions 
were neutral, the effect remained pretty well constant after excita- 
tion of the field. On the other hand for acid solutions (which con- 
tained only very little free acid) a diminution and a reversal of the 
effect soon took place, till a value was reached, about ten times as 
great as the first effect after the excitation of the field. It is remark- 
able that Rowrnanp and Beni also always found such a reversal, 
whereas Squimr found that above a certain strength of field the effect 
no longer increased, which is in agreement with what I observed. 
Another phenomenon that I regularly observed was the increase of 
the resistance of the solution as it was longer in the tube. At last this 
resistance can reach a value of some hundreds of thousands of ohms. 

Besides I made experiments with nickel. The electrodes were of 
so-called “Rein nickel” from the firm Kanrsaum; as electrolyte 
generally a 5°/, solution of nickel sulphate was used. No effect, 
however, was observed with certainty, so long as the solution was 
neutral. Probably there was an effect in the sense required by the 
theory, but about five times smaller than for iron, which would 
therefore harmonize better with the theory. It was, however, impos- 
sible to obtain certainty in this respect, as the resistance of the 
solution soon became exceedingly great, even up to more than 
10° 2; moreover the zero position was very variable, much more 
so than was the case for iron, It is peculiar that the large resistance 
only consisted for very small electromotive forces; if on the other 
hand the latter was a few volts, the resistance became only a few 
thousands of ohms. For solutions of nickel sulphate greatly acidified 
with sulphurie acid no other effect was found than in neutral 
solutions ; there was no question of a reversal here, 


760 


Physics. — “Further experiments with liquid helium M. Prelimi- 
nary determination of the specific heat and of the thermal 
conductivity of mercury at temperatures obtainable with liquid 
helium, besides some measurements of thermoelectric forces 
and resistances for the purpose of these investigations’. By 
H. KamernincH Onnes and G. Houst. Communication N°. 142¢ 
from the Physical Laboratory at Leiden. 


(Communicated in the meeting of June 27, 1914). 


§ 1. /ntroduction. Measurements of the specific heat and of the 
thermal conductivity of mercury were considered to be of special 
importance with a view to the discontinuity, found at 4°.19 K. in 
the galvanic resistance of this metal. The preliminary results have been 
already mentioned in Comm. N°. 133, for the measurements were 
carried out as early as June 1912. We wished to repeat the experi- 
ments, which we considered only as a first reconnoitring in this 
region, because our opinion was, that, by some improvements in the 
experiments, the accuracy of the results could be considerably 
increased. Special circumstances frustrated this, and now, as there 
seems to be no prospect of a repetition for the present, we com- 


municate the details of our investigation. 


§ 2. Thermoelectric forces. The first difficulty in these deter- 
minations was the choice of a suitable thermometer. The measure- 
ments already performed about the resistance of platinum, gold and 
mercury did not give much hope, that there would be among the 
metals a suitable material for resistance thermometers. We have 
therefore investigated a series of thermoelements. The gold-silver 
couple, a suitable thermometer at hydrogen temperatures *), showed 
down to the higher helium temperatures a fairly large thermoelectric 
power, at the lower helium temperatures, however, the thermoelectric 
power diminishes rapidly, so that this couple did not satisfy the 
requirements. Moreover, this couple was not at all free from disturbing 
electromotive forces, which appeared at places of great fall of tem- 
perature in the cryostat. Nearly all other elements were subject to the 
same fault. But apart from this, none of the combinations was suitable. 
Notwithstanding, we communicate the results of our determinations, 
because they show clearly that according to the theoretical investi- 
gations of Nernst and Kersom*), the thermoelectric power of all 


1) Compare H. Kameruingu Onnes and J. Cray, Comm, N°. 1070. 

2) W. Nernst, Theor. Chem. 7e Aufl. 1913 p. 753. Berl. Sitz. Ber. 11 Dez. 
1913 p. 972. 

W. H. Kessom, Leiden. Gomm. Suppl. N°. 30) (Proceedings May 1913), 


761 


couples investigated approaches to zero at heliumtemperatures. The 
different wires were measured against copper. After a preliminary 
research, which included also the determination of the thermo- 


0, 
107 


+1309 2° 


= 499! 


~400 


~ $00 


— 600 


{00 


Fig. 1. 
electric forces of nickel and of six gold-silver alloys, the following 
combinations were selected as most promising for investigations in 
liquid helium. 


Thermoelectric forces against copper. 
: | 
i Ag Au | Au, | Pt Pb Fe | Const. | VIA} 
| 
SS SaaS SS SS a paige = ie, — ——— = = 7 

81° K.| —28 S78) | S257) —298 | —457 | --1293 | —5320 | — 432 
{en ate ae He 

20° —28 | —282 | —326 —68 | —553 | +1319 | —6280 | —819 

| 4°26 —21 | —375 | —328 —58 —559 | +1309 | —6630 | —990 
| | ‘¢ eg wulbas 

3°20 aed — 383 — —59 | — +1309 | —6630 | — 1002 
— : 7 4 Li se aE = | 

| 2096 == Sone eS = = _ =) Si 1004 


“1 Aw with 0,476 weight °/) Ag. 


Figure 1 shows thew thermoelectric forces against copper, at the 
absolute temperature 7’, given in the first column of the table. The 
temperature of the second juncture was 16° C. 


§ 3. Change of the resistance of alloys with temperature. As it 
appeared impossible to find a suitable thermo-couple, our attention 
was drawn to the change of resistance of constantin, which had 
already been measured at hydrogen temperatures by KamprLINGH 
Onnes and Cray. This alloy shows bere a considerable decrease 
of resistance at decreasing temperature; it was, therefore, probable 
that constantin could be suitably used as a resistance thermometer at 
helium temperatures. Experiments have shown that this was in fact 
the case. Later measurements (see comm. N°’. 142a § 4) proved that 
also. manganin, whose resistance begins to diminish at decreasing 
temperature and which has at oxygen temperatures a considerable 
smaller resistance than at ordinary temperatures, is fit for tempera- 
ture measurements in liquid helium. 


§ 4. Specific heat of mercury. a. Experimental arrangements. 

The method, used in the determination of the specifie heat, 
agrees most with the one used by Nernst in his investigations 
about the specific heat. A little block of solid mercury hung freely in 
a high vacuum and was heated electrically. The increase of temperature 
was determined by means of a constantin resistance thermometer. 
To obtain the little block of mercury the liquid metal (comp. fig. 2 
with magnified fig. of details) was poured into the vessel C through 
a capillary, provided with a funnel, which could be introduced 
through m. First C was in the same way supplied by means of a 
funnel with a small quantity of pure pentane, which, at the intro- 
duction of the mercury, remains as a thin layer between the glass 
and the mercury. A little hollow steel cylinder (thickness of the 


wall '/,, m.m.), which contained the heating wire — a constantin 
wire, insulated with silk and covered with a thin layer of celluloid 
to avoid all electrical contact with the mercury — was immersed 


in the mercury. Round this cylinder a second constantin wire was 
wrapped, which was to be used as a thermometer. The little cy- 
linder was, by means of silk wires (stiffened by celluloid) fixed to 
a little glass rod, which could be moved up and down through 
the tube 4, and which was centred by constrictions in this tube. 
This glass rod was connected to a silk wire, which could be 
screwed up and down by turning the handle A. Now the mereury 
was frozen by cooling down to the temperature of liquid air, The 


Fig. 2. 

possible, that the results are accurate to about 10 HRs 
The thermat capacity of the hollow steel cylinder with the thermo- 
meter and the heating wires was determined afterwards by a separate 


763 


Sen 


Fig. 3. 


thin layer of pentane, which is 
spread over the glass, acts as a 
viscous lubricant at this temperature 
and prevents the sticking of the 
mercury to the wall in freezing. 
After having been frozen, the little 
block ofsolid mercury was screwed 
up by means of the handle K 
and the temperature was increased 
to about — 50° C. Thereupon a 
high vacuum was established by 
means of a GAEDE mercury pump 
and the pentane was distilled off 
into a tube, immersed in liquid air. 
During the experiments the heat 
insulation of the block appeared 
to be so good, that the tem- 
perature remained many degrees 
above that of liquid helium, al- 
though it was let down against 
the glass wall. Therefore a little 
gas had to be admitted in order 
to eool the block. This manipula- 
tion sueceeded perfectly, but the 
gas could not be removed quickly 
enough in the short time available 
for the experiments. The loss of 
heat of the mercury was thus 
very considerable (decrease of the 
temperature difference to half of 
the original value in about JOO 
seconds) and therefore the cor- 
rection, to be applied to the in- 
crease of temperature while heat- 
ing, remains the greatest source of 
uncertainty. Nevertheless it seems 


experiment, Fig. 3 shows the apparatus used for this purpose. 
b. Results. Measurement at the boiling point of helium. The quantity 
of heat supplied to the mercury amounted to 1,10 cal., the increase of 


"64 


temperature, corrected for the loss of heat during the period of heating, 
was 2,22 degrees K. whilst the quantity of heat, necessary to heat the 
little steel cylinder with the thermometers 2,22 degrees, amounted to 
O.11 cal. (result of a separate experiment). Control experiments showed 
that the heating wire (used as a thermometer). and the thermometer 
wire outside the steel cylinder had the same temperature. The mass 
of the mercury was 314 erammes, so that 0,00142 cal./degree K. was 
obtained for the mean specific heat between 4°,26 K. and 6°,48 K. 

The relation of GRUNEISEN ') = = c, would”) have given ¢,=0.0087, 
for 4°.27 K. 

Measurement at 3°.5 K. Afterwards the experiment was repeated 
at the temperature of liquid helium, boiling under a pressure of 6 em. 
of mereury ; 0.000534 cal./degree K. was found for the mean specific 
heat between 2°93 K. and 3°97 K. 

Assuming this mean value of the specifie heat, we shall calculate 
now the value of this quantity for a definite temperature according 
to Desue’s formula, which holds for our very low temperatures 

c= C.T?, 
so that the mean specific heat between two temperatures 7’, and 
[aS 
ee Uh 0) 
GSI) 

We obtain from the two experiments C= 0.0000088 and 0.0000127 
respectively. 

The agreement is not satisfactory; although, taking into account 
that the absolute temperature occurs in the formula in the 4" power, 
and that therefore small deviations in 7’ involve very large ones 
in (, we may safely conclude from our experiments, that, ith 


respect to the specific heat, nothing peculiar happens at the point of 
discontinuity, and that we may content ourselves with a preliminary 
mean value C= 0.0000110, when we assume for the moment that 
the specific heat does not show any discontinuity at all. 

We have then 

== Cit — 1010 0.000 0e* 
or for a gramme-molecule 
c= 0.00220 T?. 
For the characteristic constant 6, introduced by Drsue we find 
1) KE. Griersen, Verh. d. Deutschen Phys. Ges. 1913 p. 186. 


*) Compare KamertincH Onnes and Hotsr, Leiden Comm. N°, 142a@ Proceed. 
June 1914. 


with c, = 5.96 and 
13 3 


C= 0:00220 7 2 = 77-988 —— ce = 464 — 
ge “ 


C= 60: 

As a matter of fact, the specific heat has been determined here 
at constant pressure and not at constant volume. In the foregoing 
calculation, the difference of the specific heats ¢, and ¢,, given by 

Gy 6, — Aca 
has been neglected. Indeed, A is about 7,2.10—° and c, and T ave 
both small. 

Using Desur’s formula, we can compare our results with 
those of Potuitzer'’ at somewhat higher temperatures. For this 
purpose we calculate a value of 6 agreeing as well as possible 


c 
with Poniirzer’s figures of —, we find then 110. In fig. 4 c, is 
c 


“ 
plotted as a function of 7’ according to Drie; the values, deter- 
mined experimentally, are indicated by circles. 

The accordance at helium temperatures is bad, as could be_ 
expected in consequence of the difference between the value of @ 


used in the calculation, and the one deduced from our experiments. 


b= are = ta if 
C, 
© EC = 

Se cast eae 
a7 A all | 

Qs d 

IAS | 

fe) 
o LO = 
fe] RV ae Cv SQ JOO dso 


Fig. 4. 


1) See F. Poxtirzer. Zeitschr. f. Elektrochem. 1911. p. 5. 


766 


Meanwhile we remark, that in Po.iitzer’s experiments too a distinet 
deviation from Drsiwn’s curve is to be noticed, in the sense of a 
decrease of @ (about 115—162) with decreasing temperature, which 
would be, according to our experiments, very considerable down to 
helium temperatures ; further that, according to LinprMann’s formula 
and by comparison with lead (88), 661 is to be expected for 
mercury. 


§ 5. The thermal conductivity. 

The thermal conductivity was determined by means of the appa- 
ratus, represented in figure 5. A U-shaped tube, with double 
walls, and closed at ene end, was provided . 


NG with mereury. The closed branch contained 
Shaan a constantin wire S, insulated by means 
of celluloid, which made contact with the 

a mercury at the free end. This wire’ was 

5 used as a heating wire. The current return- 

ein ed through the mereury itself by means 

of a wire, in contact with the mercury at 

M8 the open end of the tube. The fall of tem- 


perature was measured with 38 constantin thermometers 7’, 7, 
and 7’, consisting of wire of '/,, mm. thickness, wrapped around 
a small glass tube. The experimental arrangement is further ex- 


plained by the diagrammatic figure. All wires were connected to 
each other by two wires, insulated by thin layers of celluloid and 
further running free through the liquid helium. 

In consequence of a wrong manipulation during the preparation, 
the tube had lost a little mercury, so that only the two lower 
thermometer wires could be used. The heat developed in the heating 
wire and the difference in temperature thus produced were measured 
at two different temperatures, the one above and the other one 
below the point of discontinuity in the electrical resistance. The 
section of the cylinder of solid mercury amounted to 0.47 em’, 
the distance of the thermometers to 5,0 em. 

At the boiling point of helium the supplied energy was 0,633 
watt/sec., the difference in temperature produced 0.58; at 3°7 K 0,0365 
watt sec. and 0,23. 

From this we find for the mean thermal conductivity between 
4°.5 K and 5°,1 K. £=0.27 cal/em. sec. and between 3°.7 K and 
3.9 K: £=040 cal/em. sec. 


The thing, which immediately strikes us, is that there is here no 


767 
distinet discontinuity as was found at 4°.19 K in the electrical con- 
ductivity, although the thermal conductivity becomes much larger, 
when the temperature decreases. As there do not exist direet deter- 
minations for solid mercury, we only can make a rough estimation 
with the aid of Wirpemann and Franz's law. 

At the melting point, the electrical conductivity of liquid mercury 
amounts to 1.10. 10° em. 2~'and of solid mercury to about five times 
as much, thus to 5.50. 10* em—! 2~!. From this we find by comparison 
e.g. with lead about 0.075 for the thermal conductivity. The values 
here obtained in liquid helium are 3.5 and 5.5 times as large. 


Chemistry.  “Hqwilibrie in ternary systems’. XVII. By Prof. 
SCHREINEMAKERS. 


(Communicated in the meeting of Oct. 31, 1914). 


Now we will consider the case, mentioned sub 3 (XVI), viz: 
the solid substance is a binary compound of a_volatile- and a 
non-volatile component. A similar case occurs for instance in 
the system Na,SO, + water + alcohol, when the solid phase is 
Na,SO,. 10H,O,; or in the system FeCl, + HCI + H,O, when the 
solid phase is one of the hydrates of ferric chloride, for instance 
Fe,Cl, .12 H,0. 

For fixing the ideas we shall assume that of the three compo- 
nents A, B, and C (fig. 1) only A and C' are volatile, so that all 
‘fapours consist either of A or of C or of A+ C. 

In fig. 1 CAde represents a heterogeneous region L—G; ed is 
the liquid eurve, CA the corresponding straight vapour-line. The 
liquid d, therefore, can be in equilibrium with the vapour A, the 
liquid e with the vapour C' and each liquid of curve ed with a 
definite Vapour of AC. 

Previously (XVI) we have seen that this heterogeneous region 
L—G can arise in different ways on decrease of pressure, viz. either 
in one of the angiepoints A and ( or in a point of AC; also two 
heterogeneous regions may occur, the one in A and the other in C, 
which come together on further decrease of pressure somewhere in 
a point of AC. 

In fig. 1 we may imagine that the region L—G has arisen in these 
different ways; curve ed may of course also turn its convex side 
towards AC. Besides this heterogeneous region 1—G' we also find, 
in fig. 1 the saturationcurve under constant pressure of the binary 
: dk 


Proceedings Royal Acad. Amsterdam, Vol. XVII. 


768 


substance /’, represented by pg [we leave the curve rs, drawn in 
the figure out of consideration for the present]. 


A 


Fig. 1. 


In the same way as we have acted in the general case | fig. 11 (1) | 
or in the peeuliar case (XI), we may deduce also now the different 
diagrams. 

T< Ty. At first we take a temperature 7’ lower than the 
minimummeltingpoint 7’ of the binary compound /. Now we tind 
a diagram just as fig. 2 for the saturationcurve under its own vapour- 
pressure of / and the corresponding straight vapour-line.  In_ this 
figure, in which the component-triangle is only partly drawn, Agn 
is the saturationcurve under its own vapourpressure; we find the 
corresponding straight vapour line Cy, on side CA. 

When we assume, as is supposed at the deduction of fig. 2, that 
neither a point of maximum-pressure, nor a point of minimum- 
pressure occurs, the pressure increases from m towards h; conse- 
quently it is lowest in n and highest in 4, without being, however, 
a minimum in 2 or a maximum in hk. It follows from the deduction 
that the sides solid-gas and_ solid-liquid of the threephasetriangles 
must be situated with respect to one another and to the side CB 
just as is drawn in fig. 2. 

It is apparent from the figure that the binary liquids 1 and 7 ean 
be in equilibrium with the unary vapour C' and that the ternary 
liquids a, c and #4 ean be in equilibrium with the binary vapours 


a,, c, and #,. It is apparent that somewhere between the liquids c 


1 
and 4 a liquid g must be situated, the corresponding vapour g, of 
which represents the extreme point of the straight vapour line Cg,. 

When a liquid follows curve /n, first from / towards g¢ and after- 
wards from g towards n, the corresponding vapour g, follows conse- 


769 


quently first Cy, from C towards g, and afterwards again this 
same line, but in opposite direction, consequently from g, towards C. 


Fig. 2. 


Kach vapour of this straight vapour line Cy, can, therefore, be in 
equilibrium with two different liquids, the one of branch hy and the 
other of branch gn. 

We may express this also in the following way: when we have 
an ‘equilibrium /’-+- Z + G, then there exists under another pressure, 
also an equilibrium + 7,+.G,, in which Z and ZL, have a 
different composition; G and G,, however, have the same composition. 

It is apparent from the deduction of fig. 2 that in curve jn also a 
point of maximumpressure can occur. This case is drawn in fig. 3; 
in represents again the saturationcurve under its own vapourpressure 
and Cy, represents the corresponding straight vapourline; M7 is the 
point of maximumpressure, J/, the corresponding vapour. The points 
M,, M, and F must of course be situated on a straight line. 

While under the pressure Pj; there occurs only one equilibrium, 
viz. f+ Lip+ Gau,, under each pressure, somewhat lower than 
P\, there exist two equilibria, for instance + L, + Gi, and 
F+ L,+ G.,.; we can imagine these to be represented by the 
threephasetriangles Maa, and /cc,, when we imagine both triangles 
in the vicinity of the line #//,. It follows from the deduction 
of the diagram that both these triangles turn their sides solid-gas 
towards one another, consequently also towards the line /J/M,. 

Suppose, we want the curves ed and pg to move in fig. 1 with 
respect to one another in such a way that a point of minimum- 
pressure occurs on the satnrationcurve under its own vapourpressure, 

51* 


770 


then we see that this is impossible. Yet we can imagine a saturation- 
eurve with a point of maximum- and a point of minimumpressure. 


When we trace curve /n starting from n, we arrive first in the 
pot of maximura- afterwards in the point of minimumpressure. 
We will refer to this later. 

Tp < T. Now we take a temperature 7’a little above the minimum 
meltingpoint 7p of the solid substance /#. Then we must distinguish 
two cases, according as the solid substance expands or contracts on 
melting. We take the first case only. 

Then we find a diagram like fig. 4 (XI); herein, however, the 
same as in figs. 2 and 3, we must imagine that the vapourcurve 
han, is replaced by a straight vapourline Cg, on side CA. We 
will refer later to the possibility of the occurrence of a point of 
maximum- and a point of minimumpressure. 

We can, however, also get curves of a form as curve /nand the 
curves situated inside this in fig. 6 (XI); these curves show as well 
a point of maximum- as a point of minimumpressure, 

When we draw the saturationcurves under their own vapour- 
pressure for different temperatures, we can distinguish two prineipal 
types; we can imagine those to be represented by figs. 5 (AI) and 
6 (XD. At temperatures below 7'p these curves are circumphased, 
above Z'p they are exphased. In tig. 5 (XI) they disappear in a point 
H on side BC, in tig. 6 (XI) in a point A within the triangle. The 
corresponding straight vapourlines disappear in fig. 5 (XI) at 7 in 
the point C; in figure 6 (XI) they disappear at 7 in a point R,, 
the intersecting point of the line /’R with the side CA. 


771 


Now we will consider some points more in detail. In order to 
get the conditions of equilibrium for the system #’+- 4 + G, when 
Fis a binary compound of 6 and C and when the vapour consists 
only of A and C. we must equate «=O and y,=0. The conditions 
(1) (II) pass then into: 


Z OZ 


Ew 
Mite he Cig ge ae az az, | 
: 0%, | 02 _, Ow ae, | ) 
ae” og, tb Sanur = 


Now we put: 
b= Was ikititird pnol A SG Je iii lon 5 2 (P) 
Hence the conditions (1) pass into: 


OU 0U 
«—+(y — 8)—+ RTe—U+S5=0... . (8) 
Ow 7 Oy 
aU. oo 
#,—— —6— + RTx, —U,+5=>0... . (4) 
Ow, Oy 
0U aU, ? 
— + RT logx =——+ RT loge, . . . . . (5) 
Ow Ox ; 


1 
When we keep the temperature constant, we may deduce from 


(5): 
[er + (y — B)s + RT) dz + [as + (y—A)t]dy=AdP . (6) 


(3) 


E — ps + “ rr | dx + [#,s — Bt]dy =(A+ C)dP. . (7) 


RL RT OV OV 
r + —— | da + sdy — (» + —— | dz, =({| —— — ]dP . (8) 
2 2X, Ox, Ow 


i 


Here we must equate of course in A and C a=O and y, = 0. 
In order to let the pressure be a maximum or a minimum, dP 
must be = 0. From (6) and (7) it follows that then must be satisfied : 

ip [o) a= Gann) ==, ato ogo co oe A) 

This means that the point of maximum- or of minimumpressure 
M (x,y) and the corresponding vapourpoint J/, (v,y,) are situated 
with / on a straight line (fig. 3). 

In order to examine the change of pressure along a satuyration- 
curve under its own vapourpressure in its ends / and n (figs. 2 and 3) 
we equate in (6) and (7) e=0 and a, =U. Then we find: 


OV 
[(y—B) s + RT] de + (y—p) tdy = | v- v + (B—y) F | dP (10) 
OY 


ae “ OV 
— ps + — RT | dx — ptdy =| V, —v + 8 a CLE es (Lal) 
: y 


772 


The ratio v,:2 has a definite value herein, as it follows from (5). 
When we eliminate dy from (10) and (11), then we find: 


[2+ a | era =[3V + (y—B) V, — yx] dP. . (12) 


The quantities in the coefficient of dP relate all to the binary 
equilibrium # + £-+ G. When we eall AV, the change of volume, 
when between the three phases of this binary equilibrium a reaction 
takes place, at which the unity of quantity of vapour arises, then is: 

(y—B) AV, = BV + (y—8) VV, — yo «.. « «= (18) 

Consequently we may write for (12): 


pe SA ela 14 
Ni — aura Ame mere es. 5, (124) 


Now we introduce again, as in (XI) the perspective concentrations 


of the substance A in liquid and gas; it is evident that the per- 
spective concentration S, is equal to the real concentration «, of A 
in the vapour; we find for the perspective concentration of A in 
the liquid: 
fa a 
p—y 


so that we can write for (14): . 


dP ie S\ RL 
é = —/{ 1 — — |—— .w sz 2 (th) 
aa ) c—0 x x, Ay : 


When the vapour contains the three components, then. as we have 
seen previously (14) (XI) is true; when we replace herein S, by 2,, 
this passes into (16). 

It follows from (16) that the sign of the change of pressure in 
the ends / and n of a saturationcurve under its own vapourpressure, 
depends on the sign of AV,. Now AV, is almost always positive 
for the binary equilibrium PLELG and it is only negative between 
the points / and H'|fig. 5 (XI) and fig. 6 (X1)]. Consequently AV, 
is positive in the points 4 and m of figs. 2 and 3, also in the point 
h of fig. 5 (XI) and 6(X1I); AV, is negative in the point n of the 
two last figures. Further it follows that the sign of the change of 
pressure is not determined by the ratio «,:a (the partition of the 
third substance between gas and liquid) but by the ratio S: a, (the 
perspective partition of the third substance between gas and liquid). 

Let us take now a liquid of the saturationcurve under its 
own vapourpressure in the vicinity of the point / of fig. 2, for this 
we imagine triangle Maa, in the vicinity of the side LC. From the 
position of Fa and Fa, with respect to one another, follows 


773 


S>z2x,. As AV, is positive in fh, it follows from (16) that the 
pressure must decrease on addition of a third substance. We see 
that this is in accordance with the direction of the arrow in the 
vicinity of h. 

In the vicinity of point / of fig. 3 is a, > S as follows from the 
position of triangle Kaa,. As AV, is positive, it follows from (16) 
that the pressure must increase on addition of a third substance. 
This is in accordance with the direction of the arrow in the vicinity 
of fh. 

In the vicinity of point n of the figs. 2 and 3 S is negative (we 
imagine for instance in fig. 2 triangle /6/, in the vicinity of side 
BC); as AV, is positive, it follows from (16) that in both figures 
the pressure must increase, starting from n. 

Consequently we find: in a terminatingpoint of a saturationcurve 
under its Own vapourpressure, situated between Cand H, the pressure 
decreases on addition of a third substance, when the threephase- 
triangle turns its side solid-gas towards LC (fig. 2) and the pressure 
increases when the threephasetriangle turns its side solid-liquid 
towards BC. 

As, therefore, at temperatures lower than 7'p (figs. 2 and 8) the 
pressure always increases, starting from 7, and increases or decreases 
starting from /, we find the following. When we trace curve nh, 
the pressure increases continually starting from » towards / (fig. 2), 
or we come starting from 7 first in a point of maximumpressure, 
after which the pressure decreases as far as in / (fig. 3) or we come, 
starting from 7 first in a point of maximum- and afterwards in a 
point of minimumpressure, after which the pressure increases up to /. 

As in point / of fig. 5 (XD the pressure decreases starting from 
h, consequent it is assumed here, that the threephasetriangle furns 
its ‘side solid-gas towards BC. (Cf. fig. 2 and fig.4 (XI); in this 
Jast figure we imagine however curve /,n, on side CA). In the point 
h of fig. 6 (XI) is assumed that the threephasetriangle turns its side 
solid-liquid towards BC. 

Let us consider now the terminatingpoint 7 of the saturationcurve 
in fig. 5 (XI) and fig. 6 (XI). As n is situated between F and H, 
AV, is negative, when the threephasetriangle turns its side solid- 
gas towards BC, then is S>.2, and it follows from (16) that the 
pressure increases on addition of a third substance. We then have 
the case of fig. 5 (XI). When, however, the threephasetriangle turns 
its side solid-liquid towards LC, then S<.w, and it follows from 
(16) that the pressure decreases on addition of a third substance, 
We then have the case represented in fig. 6 (XI). 


774 


When we consider the saturationcurve going through the point 
F in fig. 5 (XI) and fig. 6 (XI), then for this point y=, conse- 
quently, according to (15) S=o. From (13) follows also AV,= @. 
Therefore we take (12); from this follows for y= 8 


dP th 17) 
de tar eee Ge ee ( 


As fig. 5 (XI) and fig. 6 (XT) are drawn for V > v, the pressure 
must increase starting from / along the saturationcurve going 
through F. 

As the pressure increases starting from /’ along the saturation- 
curves under their own vapourpressure of fig. 6 (XI) and decreases 
starting from a point , situated in the vicinity of H, somewhere 
between /’ and n must consequently be situated a point, starting 
from which the pressure neither increases nor decreases. This point 
is, therefore, the point of maximum- or of minimumpressure of a 
saturationcurve, and is not situated within the componenttriangle, 
but accidentally it falls on side LC. It follows from the figure that 
this point is a point of minimumpressure; we shall call this the 
point m. 

The limiteurve (viz. the geometrical position of the points of 
maximum- and minimumpressure) goes consequently through the 
points m and R&R; it represents from m to & points of minimum- 
pressure; starting from / further within the triangle, it represents 
points of maximumpressure. This latter branch can end anywhere 
between /7 and C' on side BC. 

The terminatingpoint of a limiteurve on side SC’ can be situated 
between “and C, but cannot be situated between /’and B. A similar 
terminatingpoint is viz. a point of maximum- ora point of minimum- 
pressure of the saturationcurve, going through this point. Consequently 
in this poimt along this saturationcurve dP=0O,; from (16) it follows 
that then must be satisfied : 


S=2,. or, Pe - (y—S) ac, 0, eee eremea (l) 


Herein w and «, are infinitely small; their limit-ratio is determined 
by (5). As 2 and a, are both positive, it follows from (18): y < ~. 
The terminatingpoint of a limiteurve must, therefore, be situated 
between /’ and C' (fig. 6) and it cannot be: situated between / and 
B. In accordance with this we found above that one of the ends 
of the limiteurve is situated in fig. 6 (XI) between n and PF, 

Now we must still consider the case mentioned sub 4«(XIV), viz. 
that the solid substance is one of the components. A similar case 


775 


occurs for instance in the systems: 7+ water + aleohol, wherein 
Z represents an anhydrie single, salt, which is not-volatile. 

For fixing the ideas we assume that B is the component, which is 
not-volatile (fig. 1), so that A and C'represent the volatile components. 

Now we imagine in. fig. 1 curve pq to be omitted, so that the 
curves ed and rs rest only, ed is the liquideurve of the region L —G, 
rs is the saturationcurve under a constant pressure of the substance B. 

We can, in order to obtain the different diagrams, act in the same 
way as we did before in the general case, or as in communication 
XI. For this we consider the movement of the curves ed and rs 
with respect to one another on decrease of pressure. 

As we assume that A is not volatile, these considerations are 
not true, therefore, for points situated in the vicinity of B. Equilibria 
situated in the immediate vicinity of B have viz. also always the 
substance 4 in their vapour, so that the considerations of com- 
munication XIII apply to these. 

When we decrease the pressure, the liquideurve ed (fig. 1) shifts 
further into the triangle towards the point 4, so that under a definite 
pressure the curves ed and rs meet one another. Now we distinguish 
three cases. 

1. We assume that the curves ed and 7s meet one another first 
in a point on one of the sides of the triangle; when this takes place 
on side BC, then consequently the points e and 7 coincide in fig. 1, 
while the two curves have no other point in common further. On 
further decrease of P, this intersecting point shifts within the triangle 
and it disappears at last on the side A, when in fig. 1 the points 
s and d coincide. Curve ed is situated then inside the sector Brs 
and curve 7s inside the region CedA. . 

From this follows that the saturationcurve of B under its own 
vapourpressure can be represented by curve habn in fig. 4, in which 
the arrows indicate the direction, in which the vapourpressure increases. 
The corresponding vapourcurve is the side CA; the liquid / viz. is 
in equilibrium with the vapour C, liquid n with the vapour A and 
with each liquid (a and 6) of in a definite vapour (a, and 6,) of CA 
is in equilibrium. It follows from the deduction that the threepbase- 
triangles (Bua,, bbb,) turn their sides solid-gas towards the point / 
and their sides solid-liquid towards the point 7. 

This fig. 4 is a peculiar case of fig. 2 (XIII); when we suppose 
viz. that the substance 6 does not occur in the vapour, curve h,a@,b,7, 
of fig. 2 (XIII) must coincide with the side CA of the triangle and 
fig. 4 arises, 


2. Now we assume again that the curves ed and rs (fig. 1) meet 
one another first in a point of the side BC; this point of inter- 
section shifts then on further decrease of P into the triangle. Under 
a definite pressure we want a second point of intersection to be 
formed by the coincidence of d and s (fig. 1). The two points of 


B 
\ 
C44 doe 
Fig. 5. 


intersection approach one another on further decrease of pressure, 
in order to coincide at last in a point m. It is evident that m is a 
point of minimumpressure of the saturationcurve under its own 
vapourpressure; if is represented in fig. 5 by curve wambv, the 
corresponding vapourcurve is the side Cd. It is evident that the 
vapour m,, which can be in equilibrium with the liquid m, is 
situated on the line Am. 

3. We can assume also that the curves ed and rs (fig. 1) meet 
on decrease of pressure first in a point J/, which is situated within 
the triangle. On further decrease of pressure then two points of 


Tae 


intersection arise; the one disappears on BC by the coincidence of 
e and 7, the other on LA by the coincidence of d and s (fig. 1). 
It is evident that J/ is then the point of maximum-pressure of the 
saturationcurve of 6 under its own vapourpressure, the corresponding 
vapourpoint J/, is situated of course on the line JZ. 

One can understand the occurring diagram with the aid of fig. 5 ; 
herein we have to give an opposite direction to the arrows and we 
have to replace the points of minimumpressure m and m, by the 
points of maximumpressure Jf and J/,; further the triangles Baa, 
and bbb, are to be drawn, in such a way that they turn their 
sides solid—gas towards the line BILM,. 

We shall consider some points in another way now. In order to 
find the conditions of equilibrium for the equilibrium 6 -+ LZ + G, 
when the vapour consists of A and C only, we equate in the 


relations (1)—(8) @=1; in the general values of A and C (II) 
we put c= 0, B=1 and y, = 0. The condition for the occurrence 
of a pot of maximum- or of minimumpressure (d= 0) becomes then : 
= (=) a 2 co 6) oso, 5 (LO) 
»lhis relation also follows from (9), when we put B=41. This 
means: the pot of maximum. or of minimumpressure of the saturation- 
curve of £6 under its own vapourpressure and the corresponding 
vapourpoint are situated with point B on a straight line (fig. 5). 
In order to determine the change of pressure along a saturation- 
curve under its Own vapourpressure in its ends on the sides bC and 
BA (figs. 4 and 5) we put in (16) B=1. We then find 


dP ie ISIN\. tase ee 
sia ae sh Ae es E00) 
dz ]y—0 au Goad (AWS 


In this S and AV, are determined by (13) and (15), when we 
put herein 3=1. Consequently S is always positive. When we 
apply (20) to the figures (4) and (5), then we see that the change 
of pressure is in accordance with the position of the sides solid-gas 
and solid-liquid of the threephasetriangles. 


Now we have treated the case that either the binary compound 
J (figs. 2 and 3) or the component / (figs. 4 and 5) occurs as solid 
phase. When /’ and #4 occur both as solid phases, then the two 
saturationcurves under their own vapourpressure can either intersect 
one another or not. We only consider the case, drawn in fig. 6, that 
the two curves intersect one another in a point; the vapour, being 
in equilibrium with the liquid s, is represented by s, (s, or s,). 

A similar case may occur for instance in the system Na,SO, + 
water + alcohol, then curve cs is the saturationcurve under its own 


778 


vapourpressure of Na,SO,.10H,O (/’), sa the saturationcurve of the 
anhydriec Na,SO, (3). Then there exists a series of solutions, saturated 
under their own vapourpressure with Na,SO,.10H,O (curve cs) 
and one series saturated with Na,SO, (curve sa); the equilibrium 
Na,SO, . 10 H,O + Na,SO, + L;-++ G, occurs only under a definite 
pressure P,. The solution ZL, has then a detinite Composition s and 
the vapour, which consists only of water and alcohol has a definite 
composition s,. 

In the binary system Na,SO, + water, the equilibrium Na,SO, . 10 
H,O + Na,SO, -+ vapour exists only under one definite pressure; we 
shall eall this pressure P,. In the ternary system Na,SO, + water + 
aleohol the equilibrium Na,SO, . 10 H,O+Na,SO,+-L.-++G, exists also _ 
only under a definite vapourpressure P.. This pressure P. is influenced 


A 


Fig. 6. 
by the watervapour and the alcohol-vapour together; now we may 


show that the partialpressure of the watervapour herein is also equal 
tio P, and that the pressure of the alcohol vapour is consequently 
P,— P,. 

In order to show this, we consider the general case that in the 
system A+ B+ C (figs. 1—6) the substances A and C are volatile 
and that a compound /° of 6 and C occurs. 

The binary equilibrium 5 -+ /-+ G,, wherein the vapour consists 
of C only, occurs under a single pressure P, only. 

The ternary equilibrium 6-+ /’+ G, wherein consequently the 
vapour consists of A and C, can occur at a whole series of vapour- 
pressures. 

When we represent the § of 45 and / by § and &,, then the 
condition of equilibrium is true: 


Z, 
5 —e=0—A) (4 — nie): Serer.) 


vars) 


Hence follows: 
j OAT on nh Oe 
v, — bv — (1 — p){ V, — 2, e dP+ (1—§8)a,r,de#,=0. (22) 
eB 


When we assume that the gas-laws hold for the vapour G, then: 
Ok eee RT 
— SU 20) 3 SSS 
Oar, a,(1—2,) 
From (22) now follows: 


(23) 


l=6 
[(d —8) V, =», + Bo] dP= — 


tH) 


donee ee (24) 
1 
The coefficient of ¢@P represents the change of volume when 1 Mol. 
F is decomposed into 3 Mol 6-+ (1 — g) quantities of G; this is 
very nearly (1— 8) V’,. As at the same time PV, = RT, we can 
write for (24); 
(Al = op) CUP Sse 5 5 9 Go 6 o 4 ira) 
From this follows: 
i 0 oR 
ear MEPS we eet an (26) 
When we call the partial pressures of A and C in the vapour )4 
and Pc, then Pg=2,P and Pe=(1—a2,)P; from (26) now 
follows : 


Pea ands PG == Py) a2) 


ater 0 
l—2, 


A 

This means that in the ternary equilibrium 5+ /-+-G the partial 
pressure Po of the substance C is equal to the vapourpressure of 
the binary equilibrium 6+ #' + G,. 

When we bear in mind now that in a system the pressure and 
the composition of the vapour do not change, when we add to this 
system stili a liquid, which is in equilibrium with all phases of this 
system, then follows: 

In the ternary equilibria B+ F+G and 6+ F+ L,+ G, the 
partialpressure of the substance C in the vapour is equal to the 
vapourpressure of the binary equilibrium 4+ + G,. 

The first equilibrium (viz. 5+ /’+ G) exists at a whole series 
of pressures; both the others oecur under a definite pressure only. 

The binary equilibrium Na,SO .10H,O + Na,SO, + watervapour 
has at 25° a vapourpressure of 18.1 m.m. when we add alcohol, 
then, when the gas laws hold in the vapour, in the equilibriam 
Na,SO,.10H,O + Na,SO, + G and Na,SO,.10H,O + Na,SO, + L+G 


the partialpressure of the watervapour will also be equal to 18.1 m.m. 


Now we will put the question, whether we can also deduce some- 


780 


thing abont the change of pressure starting from s along the curves 
sa and sc (fig. 6). In communication V we have deduced the following 
rule. When the equilibrium solid + Z ean be converted with increase 
of volume into solid + L’ + G’ (in which ZL’ differs extremely little 
from £) then of a threephasetriangle solid—liquid—gas the side 
solid—liquid turns on increase of pressure towards the vapourpoint 
and it turns away from the vapourpoint on decrease of pressure. 

When we assume now that s (fig. 6) is not situated in the vicinity 
of B or F (the equilibrium 5-+ L and + LF converts itself into 
B+ L’+ G6’ and &+ L’+G" with increase of volume) we can 
apply the above-mentioned rule. We distinguish now according as 
the vapour is represented by s,,s, or s,, three cases. 

1. The vapour is represented by s,. 

First we consider the threephasetriangle /’ss,. When the side Fs 
turns towards c, then consequently it turns towards its vapourpoint 
s,; the vapourpressure increases, therefore, starting from s along ‘sc 
towards ec, 

Let us consider now the threephasetriangle Lss,. When the side 
Ls turns towards a, if turns, therefore, away from its vapourpoint 
s,; consequently the vapourpressure decreases starting from s along 
sa towards a. : 

Consequently we find that the vapourpressure starting from s 
increases along sc and that it decreases along sa. It is evident that 
this is only true for points in the vicinity of s; the occurrence at 
a greater distance of s of a point of maximumpressure on sc and a 
point of minimumpressure on sa, is viz. not excluded. 

2. The vapour is represented by s,. 

It follows from a consideration of the threephasetriangles /ss, 
and ss, that the vapourpressure starting from s increases as well 
along sc as along sa. 

3. The vapour is represented by s,. 

It follows from a consideration of threephasetriangles #’ss, and 
Bss, that the vapourpressure starting from s decreases along sce and 
increases along sa. 

We can obtain the previous results also in the following way. 
Between the four phases of the equilibrium 6+ #’+ L, + vapour 
or s,) a phasereaction occurs on change of volume. We choose 
this reaction in such a direction that vapour is formed, we call the 


(Si, Sq 
change of volume AV. 

The point s (fig. 6) is a point of the quadruplecurve B-+ #+ 
+L+G; AV is positive for each point of this curve. When, 
however, a point of maximumtemperature /7 occurs on this curve, 


781 


then AV is negative between this point /7 and the terminatingpoint 
of the curve on side BC. It is apparent from the position of the 
curves sc and sa (fig. 6) that point s is chosen on that part of the 
quadruplecurve, where AJ is positive. We distinguish now again 
the same three cases as above. 

1st. The vapour is represented by s,. 

It is apparent from the position of the points 7’, B,s and s, with 
respect to one another that the fourphase-reaction : 

Nee GV. S0) 

F+ L4G (Curve sc) B+ L+ G (Curve sa) 

FH+B+L FI+B+G 
takes place; it proceeds from left to right with inerease of volume 
Hence it follows that the equilibria written at the right of tbe 
vertical line occur under lower pressures, the equilibria at the left 
occur under higher pressures. In accordance with the above we find, 
therefore, that starting from s (fig. 6) the pressure increases along 
se (equilibrium + 1+ G) and decreases along sa (equilibrium 
B+L+ GQ). 

2°¢ and 3". Also in these cases we find agreement with the 
previous considerations. 

When a point of maximumtemperature H occurs on the quadruple- 
curve b+ F+ 2+ G, then two points of intersection s occur at 
temperatures a little below 77. When we consider now a point 
of intersection s between // and the terminatingpoint of the qua- 
druplecurve on side AC, then ATV’ is negative. This involves that 


above in 1st—3'4 increase of P is replaced by decrease of P and 
reversally. We find also the same when we consider the threephase- 
triangles solid-liquid-vapour. To be continued.) 
Chemistry. — “On the quaternary system: KCI—CuCt,— Ba Cl,—H, 0.” 
sy Prof. Scurememakers and Miss W. ©. pr Baar. 
(Communicated in the meeting of October 31, 1914). 


In a previous communication’) we have already discussed the 
equilibria occurring in this system at 40° and at 60°; the results of 
the analysis on which these considerations are based, we have hitherto 
not yet communicated. Now we will communicate the results of the 
analysis; all the points, curves ete. quoted in this communication 
apply to the two figures of the previous communication (1. c¢.). We 
want to draw the attention to the fact that fig. 1 represents the 
equilibria at 40° and tig. 2 the equilibria at 60°. 


1) These Communications (1912) 326. 


782 
vACE eae 


Composition of the solutions in percentages by weight at 40° (fig. 1. I.c.). 


Point KCl BaClo | CuCl, H,O | Solid phases 


a 0 0 44.67 | 55.33 Cu Cly.2H,0 
b 0 3.72 | 42.72 | 53.56 | BaCl.2H,O-+CuCl.2H,0 
c 0 28.98 0 11.02 |) Ba Cl. Hp O 
d | 23.98 | 9.15 0 66.87 BaCl).2H,0+KCI 
e | 28.63 Deg Og, [eres KCI 
f | 21.53 0 | 22.85 | 55.62 Keeper 
gz | 9.79 0 | 43.83 | 46.38 CuCl, 2H; 0- Des 
b 0 3.72 | 42.72 | 53.56 | BaCl,.2H,O +CuCl,.2H,0 
es 5.52 | 3.39 | 42.35 | 48.74 : 
“pn | 9.88 | 2.99 | 42.07 | 45.06 | BaClh.2H,O4- CuCl. 2H0°-D gs 
di VW/23508s)) V94s lao 66.87 Ba Cl,. 2H» O + KCl 
2 | 21.46 | 8.90 | 8.44 | 61.20 ? 
>| 20.61 | 7.63 | 14.31 | 57.45 | ; 
i | 20.61 | -5:40 | 20.47 | 53.52 | BaCh.2Hs0--KCI--Dioo 
f | 21.53 0 22.85 | 55.62 Ke eD ee 
a 21.31 | 2.59 | 22.06 | 54.04 f 
eel 20K | 5.40 | 20.47 | 53.52 BaCly.2H:0 + KCl + Dy.20. 
pel Sods h 43.83 | 46.38 CuCl, .2H:0 + Dy.o» 
aa 9.94 | 1.46 | 43.22 | 45.38 : 
oh 9.88 | 2.99 | 42.07 | 45.06 | CuCl. 2H,O + BaCl.2H,0+ Dhow 
i | 20.61 | 5.40 | 20.47 | 53.52 BaCly. 2H,0 + KCI+ Dig. 
2 | 16.44 | 4.72 | 27.22 | 51.62 Ba Cly 2H,0 + Dy.o.0- 
G” | q1.44 [93.65 | aales | 0.55 : 


h 9.88 | 2.99 | 42.07 | 45.06 | CuCl,.2H,O + BaCly. 2H.0 + Dj.» 


TABE ES IE 


4 ¢3 


- Composition of the solutions in percentages by weight at 60° (fig. 2 1.c.). 


Point) KCI | BaCl, CuCl, H.,0 Solid phases 
a OS... if eo 41.42 | 52.58 CuCly . 2H,0 
b 0 6.87 | 43.57 | 49.56 CuCl, . 2H,O ++ BaCly . 2H,0 
pe aaa Bi 0 68.3 BaCly . 2H,0 
@ | 23.09, | 14.83: | 0 62.08 BaCly . 2H,0 + KCl 
aa 32 0 0 68.8 KCI 
| | 
if 26.12 0 26.57 | 47.31 Kele= Dis 
@ | 17:13 | 43.45 | 39.42 Dioce Dia 
k | 13.67 0 46.40 | 39.93 CuCl, .2H,O0 + Dy. 
S | 
b o | 6.87 | 43.57 | 49.56 CuCl, . 2H.0 + BaCl, .2H,O 
v | 
ES | 6.32 | 5.99 | 43.68 | 44.01 : 
O \ 
l 12.45 4.93 44,09 | 38.53 | CuCl.2H,O-+BaCl.2H.O+D,, 
d | 23.09 | 14.83 0 62.08 | BaCl,.2H,O+ KCl ~* 
Bos 
ES | 23.15 | 10.01 | 12.01 | 54.83 | 
O 
i | 23.78 | 5.97 | 24.61 | 45.64 BaCl, .2H,O + KCl + Dj.2.0 
FA e26u 1b ee 6 26.57 | 47.31 KEleD os 
2 
Ew | 24.53 3.32 | 25.46 | 46.69 E 
a | 
i | 23.78 | 5.97 | 24.61 | 45.64 KCI + BaCly . 2H,0 + Dj.0. 
medidas |) 0 43.45 | 30.42 Dios Dix 
vu 
ES, | 16.50 | 2.51 | 42.20 | 38.79 : 
O 
h | 15.75 | 4.75 | 40.84 | 38.66 BaCly.2H,0 + Dyno + Din 
bee See) ree EE ee 
k | 18.67 0 46.40 | 39.93 Cue wZHO sa Dig 
vu 
Em | 13.04 | 2.52 | 45.24 | 39.20 i 
O 
1 | 12.45 | 4.93 | 44.09 | 38.53 | CuCl,.2H,O+ BaCly.2H,O+ D,, 
i | 23.78 | 5.97 | 24.61 | 45.64 KCI + BaCly. 2H,O + Dy.o. 
[-P) 
ES | 19.53 | 5.40 | 32.37 | 42.70 | BaCl, . 2H,O + D 1.0.5 
O | 
h | 15.75 | 4.75 | 40.84 | 38.66 BaCl, .2H,O + D, 90+ Diy 
h Msierey |) eis 40.84 38.66 BaGly. 2H30 -— Dj.o.0-F Dj. 
{Ac 760i) 483 s\) APES) [88526 BaCly.2H,O + D:., 
1 | 12.45 | 4.93 | 44.09 | 38.53 | CuCl. 2H,O+ BaCl,.2H.O+D,4 


52 


Vroceedings Royal Acad. Amsterdam, Vol, XVII. 


784 


Physics. — “On the theory of the string galvanometer of KINtTHOVEN.” 
By Dr. L.S. Ornstein, (Communicated by Prof. H. A. Lorentz.) 


(Communicated in the meeting of September 26, 1914). 


§ 1. Mr. A. C. Crenore has developed some considerations in 
the Phil. Mag. of Aug. 1914°), on the motion of the string galvano- 
meter, which cause me to make some remarks on this subject. 

For a string, immersed in a magnetic field 7, and carrying a 
current of the strength -/, the differential equation for the elongation 
in the motion of the string is 


O*y a Oy ah | JER] (1) 
— +x%x— = a — + — a6 
Or? ot Ox” 0 

in which x is the constant damping factor, a? = —, 7, is the tension 


g 
and 0 is the density. The direction of the stretched string has been 
chosen as the a-axis. For «=O and «=/ the string is fixed, so 
y =. In deducing the equation the ponderomotive force is supposed 
to be continually parellel to the elongation y, which is only approxi- 
mately true, since the force is at every moment perpendicular to 
the elements of the string (perpendicular to / and //); but if y 
may be taken small, then the equation (1) is valid. The approxi- 
mation causes a parabola to be found for the state of equilibrium 
with constant H and ./, instead of the are of a cirele, as it ought 
to be; however, the parabola is identical with a circle to the degree 
of approximation used. 

Dr. Crrnork now observes, that the equation (1) may be treated 
after the method of normal codrdinates by putting 


DD OZ OREN Seo os of IS), 


Besides the equation 1, he deduces a set of equations, the “circuit 
equations’, which give a second relation between gy; and J (from 
(1) there originates in the well-known way an equation for every 
coordinate y,). The obtained solutions will be independent, when 
the cireuit equation is true, and again their sum is a solution of the 
problem. However, from the deduction of the circuit equation it cannot 
well be seen whether this is the ease, since not entirely exact 
energetic considerations underlie this deduction. Now supposing the 
string to be linked in a cireuit with resistance /, and self-induction 
L, the circuit-equation may be easily found by applying MaxweEt.t’s 


1) Theory of the String Galvanometer of EinrHoven. Phil. Mag. Vol. 28, 1914, p. 207. 


785 
induction-equation. For in consequence of the motion of the string 


in the magnetic field the number of lines of force passing through 
the circuit changes to an amount proportional to 


Expressed in the units used by Dr. Crenore, the induction-equation 
now takes the form: 
l 


dJ “Oy } 
ij EI eal Aah eee 8 oo 
dt Ot 


0 
where /# is an external electromotive force acting on the circuit. 

§ 2. The problem of finding the vibrations governed by the 
equations (1), (3) and the condition y=O for c=O and «=/, 
can be easily solved. First, let E be O, and so the question of free 
(damped) vibrations may be put. Suppose that 

y = —p er J = Feat 
where y is a function of 2and / is a constant. Then the equations 
change into 


9 


— wf + iwxg — a 


Oe eee 
0a? fe) 


l 
0= R14 Liwl + ‘He | gd. 


0 
Hence 
l 
Oy iw 
@? — iwe*) 4 a = pda. 
( NP or dx? o(R+ Liw) ¢ 
0 
: 4 . : ; FH’iw 
Putting w* — 7x in the first member n* and Ae =p we 
have 
3 l 
2 
Ge 
n° p+ a? =s pdx. 
ie f p 
0 
This equation may be satisfied by 
n nt : 
p=Acs—x+ Bsn—2 + C 
a a 


provided that 


or 
bo 
Eo 


TS6 


“a nl a nl : 
n? C=p Asin— + — Bl 1—cos—]+ Cl). . (4) 
n a dv a 
whereas, because of the boundary conditions, we must have 
A+. C= 
nl _ nl f 
A cos— + Bsin— + C=0. 
ai a 
This gives for the frequency the transcendental equation 
nl? 
1 — cos - 
a nlooa a 
np | — = en — = = l 
n a n _ nl 
sin — 
a 
or 
een _ nl a nl 
n* sin — == || Ls — — 1 —cos : 
a a 7 a 
From this it appears immediately that we must have 
_ nl E 
Ti PC AE ta! oS (5) 
2a 
or 
¥ nl nl 20) een ; 
Ww” COS = p l COS = sin . . . . . (6) 
2a 2a n 2a 
(5) can be satisfied by 
nl 
Sica (7) 
2a 


or, hence 


. 2k ra \* 
pA all : 


As is immediately to be seen, these are the damped vibrations of 
even order, which the string can perform in the absence of the 
enrrent. It is evident that the presence of current and field have 
no influence on the vibrations of even order. [f the resistance is 
infinitely great, the constant p in the equation (6) is zero. In this 
case the equations can be satisfied by m= 0, or w =0, i.e. the 
string is at rest; and further by 


nl 
cos — = 0. 
2a 
Hence 
nl oy 1 4g 8 
Qa — (2 tL + ) 2 . . . . . . . . ( ) 


or 


787 


ae (a) 
w* — iwx = | — es) 


The frequencies arrived at are those of odd order, altered by 
current and field. For large values of R an approximate value of 


: : : Ge eas 4) 
n can easily be expressed in the form ny + je From (6) follows 


N; =n; + Has aes i 

ag Oe Ohne ane 
s being an odd number, 7 being taken zero, while for w and n, their 
values for A=o must be put. Taking x= 0, i.e. neglecting the 
air-damping in comparison with the electrical damping, we find 
sa 4H*il 


Cys 22 Le 9 
3 l Ro s°x* (9) 
In the solution, therefore, there is a damping factor of the form 
4H] 
—= t 
e Res*x? 


The influence of the damping is the less, the greater the value of 
s is. This is directly evident, for if s is great, the string vibrates in 
a great number of parts with opposite motion. The electromotive 
force generated by those parts therefore is annulled. 

In case # is small, the roots of the equation (6) are those of the 
transcendental equation 


nl 2a nl 
lcos—= — = sin = (() 
2a n 2a 
or 
2a nl 


i) eal Lin, Se ee pa Sa CMa (10) *) 


; nl . Xe ee 
The quantity >— approaches to odd multiples of —. For small values 


of A an approximate form n,--a@R can be easily indicated. Taking 
again L—0O and x =—0, we find 

2a Ko . 

PEP * 

where 7, is an arbitrary root of (10). In case the resistance is small, 


Oe Se 


all vibrations suffer the same damping. 
For @ we find 


_ nl _ n(l—a) _ ne 
sin — — sin — — sin — 
2 a a 
—— — ie 
P _ nl 
sin — 
a 


1) Compare for instance Riemann-Weser, Partielle-Differential Gleichungen, II, 
p. 129. 


hence for 


inl _ n(l—e) _ ne 
sin — — sin — sin — . 
oy de a a 
1 Se Reo on (filthy) 
7 _ nl 
sin — 
a 


The real and imaginary part of this expression satisfy the equations 
and the boundary conditions. A sum of solutions for different values 


. oc : : dy ’ ‘ 
of @ satisfies the equation. If y and “ate given for {= 0, we can 
: dt 


with the aid of the given functions find the solution. The found 
proper functions are not orthogonal, but by an appropriate linear 
substitution orthogonal functions can be obtained. If y is known, I 
can be calculated from (3). 


§ 3. It is useful to work out the problem. Using the assumption 
(2) of Crenork, we obtain for gs, the following set of equations 
(taking & and / zero): 


= AHS 
Pot ns’ Ps = SM Sal) oe (5) 
0) 
and 
21H _ Qs 
RB se 
Uv s 
where 
SITA 
n= e 
3 l 


Here s is an odd number; for even values the second member 
of (12) is zero, and the even vibrations are therefore unchanged. 
Now putting 
Ps = ay ett ‘ Ji wlagioln 
and 
AHI 1 


2 2? 
8XO Ns? —W 


i 


we find 
21 Hiw st Lh, 
a 8 


RE A 


The frequency-equation therefore is 


81 Tio _ ] é 
- = SS Me 5 on so (Ga) 


On, ~~ (n;?—o’) a 


R+ 


This trequency-equation has the same roots as equation (6), which 
if x and / have been taken O, takes the form 


wl ie ( wl 2a , =) 
@ cos — = cos — — — sin — }. 


2a Ro 2a lw 2a 
The identity of these frequency-equations can be easily shown. 
Sl H? . ; : 
Put i=h, then (6a) takes the form 
i} a al Siete Ns W 
1s hy = Se Ee — 0 
nS a? 8? (ns? —w’) 
x? 
The sum of inverse squares of odd numbers is 3 Further, 
Oo 
: Ey dat i : , 
————; therefore the first member amounts to 
c 
k ase a 1 
1——+ 8— & == (0), 
i) Pa n—w* 
For tg z we have 
22 
eo 
es a 2 
tg er? a a te ey 
ay 
where s is again an odd number, therefore we obtain 
k 2a ol 
1——-+ —kig—=0 ..... .« (14) 
oOo wil 2a 
The equation (6) takes the form 
wl k 2a ol 
@ cos 1— — + ——ktg —— eee en-au (ko) 
2 a leo? 2a 
The equations (14) and (15) have the same roots, for the vectors 
wl ‘ = 
wo and cos = do not contribute roots to (15). 
atl 
Having found the roots of (14), we can determine y. Each root 


STL 


yields a Fourter series. In the case that (=o), sin must be 


é 


combined with one frequency only. For our case we have 


a A, iw,t , sTx 
y = >, >, ——— -e sin 
$ 2 2 
s (ns?—w+’) 
1 Sa A, 1 xt 
= sin =R e co o oe re UG) 
‘ ; ; 
s l ns —W, 


The Fourier series which is the vector of A Dae must be equal 
to the function whieh in § 2 appears as the vector of the same 
exponential. This can be shown by direct development. It is apparent 
that by a given frequency all the original normal coordinates are 


790 


§ 


et into motion. For very great and very small values of R, the 
constants A in the expression (16) can easily be determined. 
~. We can also use (9) and (11). Let us write (41) in the form 


y = emt 
: nl 
cos 
2a 
and let us introduce the value of 2 from (9), we then find 
4HT?] 
nt — —— t > 
8 Nagas Ng TR nse 
—T Ros* a 1 — cos — i— sin — 
a as a 
2H tse 
where d, = ————. Separating the real and imaginary parts, we find 
Rus aC: : : 
4 FT? 
Sp aaa, 
7 Re Regs tae 


Bs 


dé, Nett Nk 
— | 1 — cos — } cos ny t + sin sin nst | As 
i a a 
J, M8 , 5 Pe 
ap | = 1 — cos — ] sinnst — sin COS Net 
R a a 


J. gv st 
( — cos ms ‘) As —sin ae B.| 
v a a : 
dy Nyt J. Nk 4 f*] 
ee) | = SS HS Ag —{ 1 — cos B, = Bene 
@) oa sre Be a = ( a a ) z Ras*ng 7 


l l 


ae % swe “y Sma 
Putting fr sin dx =a, and _ dz = bs we have 
e e 4 


0 0 


and 


ree l 
(eae SS = SE 
R 2 
l eam 2n5 SUB 4H] B 
ae As ——~ «at Os Ds San 
: 2 R i Ros*ns 
2 ; ngl ; 
For R=o we get b= — Fei Ss Therefore B.—— = bs 
2 
and A, = —a,. Putting 
Ns 
A 2 Ee ts 
a Os == 
Ns R 
) 
Bs 
(= — fit = 
iy if R 


t9L 


we have 


() = ial = capes i Bs 
Ri Ns 2k 
ls 8H*b, 
0) SS SS SS SS i OS 
R IR Res*ns 


These series are convergent, if the conditions for the ordinary 
Fourtmr.series are fulfilled. We can therefore calculate a, and P, with 
the help of the given formulae. 


§ 4. In the case # is a given function of the time, our equation 
can also easily be solved. 
a. First if / is constant, we have 
07y Oy O°, AJ 


A Ge ae ai 7 
l 
B=RJ+ | y de. 
0 


The current / and y ean be divided into two parts, the one 
depending on ¢, the other not; we indicate those parts by the indices 
1 and 2. For the first part we have 


~<a — 
ave Q 
(T= TPE 
therefore 
ay, EH 
a? ——_ —_—— 
0a? Re 


from which y, can be determined if we take into account that y, 
vanishes for «=O and «#—/. The determining of the second part 
leads to the problem treated in § 3. The solution can be used in 
order to fulfill given initial conditions. If an initial-value of J is 
given, then y must fulfill at 40 a condition following from (3). 
b. Further, we ean consider the case = EK cos pt. 
Putting 1 = 0, we ean try the solution 
y = cos (pt + B) 
J =I cos (pt + 8) 
where g is a function of v. The first equation gives 


—pp—a 


O°” os Ay 


wv 


This eqnation can be solved by 


792 


P ae, o 
G~ =A cos z a + Bsin Fa a+ C 


or according to the above 


pl 
HI mat 
) a ) 
Q=- con e— - Be «+d oo (Cl) 
Pp a oy yall a 
sin — 
a 


Introducing this result into the second equation, we obtain 


2 


Jef Ui 
Ecos pt =: RI cos (pt + 8) + —— sin (pt + B) 
OP 


Se: - +7 }.(18) 
p a p , pe 
sin— 
a 
Now take 
IN? 
= 
TET a pl a 
sin +lj=tgea 
opk p a . pl - 
sin— 
r 


then we find 


< P 2 
1—cos —1 
Jak a ip a a 3 
Ecos pt=/14/ R? + —_( —-sin—1 — +1 } cos (pt+-B-a) 


Kis P 2 pP sin ue 1 
a 


From this we find for the retardation of phase, 8 =e; and for 
the amplitude of / 
[=— 
A 
where 7 represents the square root in the second member. The 
current / being found in this way, y can be determined from (17). 
When Z does not vanish, we can suppose y and / to depend on 
er; and finally taking the real part, and following the above method 
we find the values of y and J. 
If we express y by (2), the solution can also easily be found. We 
then have 


Substituting this into the second equation of § 3 (where zero has 
been replaced by £ cos pt) we find 


793 


PRES eer ead Oy ae 5p A MRE a teeny ges eae 
psi? L s? (ns? —p?) 
from which J/ can be found. The sum in the second member can 
be put in a way analogous to that of § 3, into a form identical 
with (18). Our result does not agree with that of CreHorE (compare 
p. 214). In our solution the retardation of phase is the same for all 
vibrations, which is not the case in Crenorn’s paper. 
It may be observed that in our problem we have to do with a 


system of an infinite number of variables in which a dissipation- 
function couples the variables; for eliminating / from (12) and (13), 
we obtain 

ele uy 


Ps + 2s P= — =e 
sok s 


The dissipation /#’ takes the form 


Groningen, Sept. 1914. 


Physics. — “Accidental deviations of density and opalescence at 
the critical point of a single substance.” By Dr. LS. OrnstErn 
and F. Zernike. (Communicated by Prof. H. A. Lorentz.) 


(Communicated in the meeting of September 26, 1914). 


1. The accidental deviations for a single substance as well as 
for mixtures have been treated by SmoLucHowsk!’) and EINsTwrn *) 
with the aid of Bonrzmany’s principle; by Ornstein *) with the aid 
of statistical mechanics. It appears as if the considerations used and 
the results obtained remain valid in the critical point. SMoLUcHOWSKI 
has applied the formula found for the probability of a deviation 
to the critical point itself, and has found for the average deviation 
of density 


He has used this formula to express in terms of the mean density 


') M. Smotucuowsk1, Theorie Cinétique de l’opalescence. Bull. Grac 1907 p. 1057. 
Ann. der Phys. Bd. 25, 1908, p. 205. Phil. Mag. 1912. On opalescence of gases in 
the critical state. W. H. Kersom, Ann. der Phys. 1911 p. 591. 

2) A. Einsrernx. Ann. der Phys. Bd. 33, 1910, p. 1276. 

5) Ornstein, These Proc., 15, p. 54 (1912), 


794 


the accidental deviations in a cube, the side of which is equal to 
the wave-length of the light used in the experiments on opalescence, 

Now there is a difficulty with this formula, to which, indeed, 
lead also the considerations of Ernsruin as well as statistical mecha- 
nies when worked out in an analogous way for the critical point. 
In all these cases the mutual independence of the elements of 
volume is presupposed. Now, let there be given for the element of 


volume v the mean square of deviation viz. (n—n)*. Consider p 


equal contiguous elements of volume v,,v,, ete., in which n,,,, ete. 
particles are situated, 7,,7, ete. indicating the mean values of these 
numbers. 

Hence in the volume V=v,-+2,-+... there are N=n,-++n, +... 
particles. 
_ For the mean value of NV we have 

N= sem er we. 

subsequently 


(N — WN)? = ((n, — n,) + (n, a) SS e Pe ae 
since, the elements of volume being supposed independent of each 
other, the means of the double products vanish. So we find for the 
deviation of density that the product of volume and mean square 
of deviation must be a constant. 

Indeed the above-mentioned formula of probability for the devia- 
tions of density is so far inexact, as the terms of higher order 
appearing in if are at variance with the mutual independence of 
the elements of volume, which underlies the deduction of the fre- 
quency-law. In fact this deduction is only valid for such large elements 
of volume that these terms are no more of any influence. It is 
easily seen that this limit, above which the formula is valid, in- 
creases indefinitely in approaching the eritical point. This explains 
also mathematically the wrong dependence on v found for the mean 
deviation in the critical point itself. 

Now one could try to deduce the formula to a farther approxi- 
mation. However, also the supposition of independence of the ele- 
inents of volume is inexact in case these are small, and it would 
thus be impossible to ascertain how far the formula would yet differ 
from reality. *) 

1) A deduction of the inequalities in which the inexact terms of higher order 
do not at all appear, is given by ZeRNiky in his ‘thesis, which will shortly 
appear. As this deduction too uses the independence alluded to, the objection men- 
tioned holds here also. 

The remark of Euyster (lc. p. 1285) that there would be no principal difficulty 


795 


2. Now, in order to avoid the difficulties mentioned, it is necessary 
to take into account the influence of deviatious in the one element 
on the state in another. Let us divide the system into infinitely 
small elements of volume. A molecule is considered to lie in the 
element when its centre is situated in it. We consider an element 
dv, in the origin of coordinates. Around this element we imagine 
the sphere of attraction i.e. the region in whieh a molecule must 
lie when it is to have any influence on the state in dv,. We determine 
the numbers of moiecules for the elements of the sphere of attract- 
ion in giving the deviations »,,r, etc. from the mean number of 


molecules per unit of volume. 


We suppose the mean value of the density »,, when », etc. are 
given, to be a linear function of the deviations y, ete., i.e. we put’) 
De C eipardia falda ese 14 ke 8.0. (ll) 

Taking the mean value of », over all possible values of »,, it 


0 
appears immediately that C= 0, hence 
De ide eed O ee eehg San At ont (2) 
The coefficients 7 denote the coupling of the elements, they only 
depend on the relative coordinates, i.e. here, on «yz. That the in- 
fluence of an element, when the density is given, must be propor- 
tional to its size is immediately seen by considering the influence 
of uniting two elements in (2). 
We shall now write the sum (2) as an integral. For the density 
in the element dv dy dz we put v,,-; further, we can dispose of / 
in such a way that 7(9,0,0) =O. Then for (2) we get 


Rae 
m= {ff ise inane) Cuan we 8 Va ve (8) 


The integration may be extended here from —o@ to +m, / 
being zero outside the sphere of action *). 


7 


in extending his deduction to a further approximation, is therefore mistaken. On 
the contrary, the consideration of higher terms so Jong as the independence is 
made use of, will not lead to anything. 

1) Putling things more generally, we could write a series in Y, ete. instead of 
(1). However, for the purpose we have in view, (1) is sufficient. 

2 The quantity » can only take the values 1—adv and —adv, hence » is a 
discontinuous function of the coordinates. One might be inclined therefore, to continue 
writing a sum instead of the integral (3) and to solve the problem dealt with in 
the text with the aid of this sum. In doing so one gets sum-formulae which are 
wholly analogous to the integrals we used. However, we prefer introducing the 
integral, as the discontinuous function v has entirely disappeared from formula (6) 
only the function g appearing in it, which is continuous when the function / is 


796 


On the contrary, if », is given, > has another value for the 
surrounding elements, than if », = 0. Be in the element at xyz 
Dive SSO DOr ed a bd B 0 0 o (4) 
and let us try “to determine the function g, the function / being 
given. 
Now take the mean of formula (3), a fixed value », being ascribed 
to yp in a certain element dv, dy, dz,. 
In w, y, z, according to (4) 
Veyz = g(&@—2,, y—y,, 2—Z,, v, dv,dy,dz,). ». - . (0) 
For the first member we therefore get 
Ht, Ys 2, v,de,dy,dz,) 
as jf and g do not depend on the direction of the line joining the . 
elements. In the integral, (5) cannot be applied to the element 
dx, dy, dz,; owever, this element gives 
Di Fi (@anyan ey) cn ay az. 


Further taking g (0,0,0) zero, as it may arbitrarily be chosen, 


we get 
4 
G(@ 454 132,50, 42, dy, dz,) = [ foe#rane-sumdondin de) fey? dadydz-4- 
e/fe 
—o 


= Dif (#141921) dx, dy,dz,. 
This is true for all values of », dz, dy, dz,, hence g must contain 
this quantity as a factor, and we obtain 


ae 
G(@ 454192) =| foe, Y— Yrs © —2) f (wyz) dadydz = flz,,4,-2,) 
—o 


Now put e«—a,=6& y—y, =, z—2z,=5, and omit the index, 
then for g we get the integral equation 


+a 
a5y/,2) a [Jr +§, yt, e+) o(Sy6) d&dyd> = f(xyc). . (6) 


For g we have 
Dayz = 9(ey2) Dis ss 5 oe ee 
from which it appears immediately that 


Daye v= y(ayz) v,? Cer oS 5 ((e) 


continuous. The integral-formulae obtained in this way are easier to deal with 
mathematically, and besides the integral equation (6) has been solved, this being 
not so easily found from the analogous sum-formula. 


797 


Now let us consider more closely the coefficient of g in (8). 

Let a molecules be present in the unit of volume, then the mean 
number of molecules in dv is equal to adv. If we take dv very small, 
there may be no or one molecule in it. The chance for one molecule 


l 
is, therefore, adv; for none 1 — adv. In the first case » = Ey a, 
av 
in the latter it is — «a, thus 
z a . 
D> = — — ar 
du 
or 
Baye ee eS, Ue ete tee ee (9) 


Introducing this into (8), we find for the two elements «,y-2, and 


UY Ze 


pv. = a — Vey Ys— Yry 25—2r) : . : . : (10) 


This result can be used to indicate the values of (W—NV)? = A N? 
for any volume. 
We have 


JIN = fra 


AN? = foe dv, dv- +{{ rv. da, dy; dz, dz- dy~ dz- 


VV VV 


from which applying (9) and (10) 


AN? =aV-+a g (@s— 2x, Ys —Yry 22 —2z) daz dys dz, dz, dy- dz. 
VV 
This holds for every size and form of V. Elaborating it for a 
cube with side / the dependence on |’ is seen more clearly. Putting 
Lf — kt, = 6, Yo — Yr =, 2% — 2 = $, and integrating only for $45 
positive, by which '/, of the integral in question is found then, we get 


U az l Li 
AN* = N+ 80f {fotsnt) | { (ae dye de 
000 gus 
Ee 
ee so | (PP ($4445) + lGyt+ 8+ 55) — Sud) g ds dy db. 
000 


79S 


é +] Jay) 
AN? ap “rr 
2 = | g (ayz) dedydz — 3 {ff — gq dadydz 
N a/e/e aes e/eu l = 
oe ®, 
+1 ane 
even “77 |a°| 
3) — gda dy dz — —_q dx dy dz. 
arg) ney 


Every integral in this formula is always smaller than the prece- 
ding one. If / is large with respect to the distance for which g has 
an appreciable value, there remains only the first integral. For 
any great volume we have 


> 


= = 1+ oda dyidz ~~ =) aes) 
3. In trying to determine the function / by means of statistical 
mechanics, we meet with difficulties. Still something may be found 
about the quantities v.»- by applying the statistie-mechanieal method 
to our problem. Indeed statistical mechanics permit to introduce a 
mutual action of the elements of volume. 

We will avail ourselves of a canonical ensemble. We suppose the 
moleeules to be spherical and rigid, and to attract each other for 
distances which are great with respeet to their size. Elements small 
with respect to the sphere of attraction therefore may still contain a 
great number of molecules. But now we drop the supposition of the 
sphere of attraction being homogeneously filled for all systems (or 
at least for by far the greater part of them) *). 

In calculating the number of the various distributions, we 
must, for the potential energy of attraction, take into account the 
mutual action of the elements; whereas, in calculating the exclusion 
of definite contigurations of centres, we may neglect the fact that 
there is some correlation on the borders of the elements. For the 
dimensions of the elements have been supposed large with respect 
to the molecular diameter. 

The mutual potential energy of the » +7 molecules contained in 
an element dv, will be represented by 


in this formula » represents the number of molecules contained in 
the volume dy for the most frequent system. In this system the 
distribution is homogeneous. 


) Cf OrwsSTEIN, Toepassing der Statistische mechanica van Gipss op molekulair- 
theorelische vraagstukken. Diss. Leiden 1908, p. 43 and p. 110. 


799 


Of course, the potential energies will not strictly be the same for 
different configurations within the elements, but we shall neglect this 
complication. Further we will represent the mutual potential energy 
for the two elements o and 9 by 

== (Oa a) (Bhat T2) Pos 
does: xt Hi 
all elements of volume being put equal. 
For the total potential energy we find, in this way 


l 
ey aT Sines ee 
oa +- %) &_(Y + To) cr. 


For the frequency §¢ of a system with the given distribution of 
molecules we find 


les 2 » 
nf ——— Selves) Sp Wr) os 
F(——  — Or dV) Ee «(o, dV y IT p2Odv ‘ 
(v1, Ww-tr, Hie 


Here w is the function defined in the quoted dissertation on p. 48. 


Supposing & & py and developing, we get, 


1 1 Ila) 1 Loy ! 
— na Pee § (— a gee si et 


S—C wr a-” e Y vp da da Odv 


The number of molecules per unit of volume represented there 
by n, has been put @ in this paper. The function @ and the faculties 
are developed in the same way as in the quoted dissertation. The 
double sum in the exponent gives the forms +.» u1-y7.,and +12 ry... 
These forms are identical, as they consist of the same terms differ- 
ently arranged, further 2y., is the same for all molecules and 
Yt. = 0, consequently both sums vanish. 


The constant C' contains the factor / Tew/O 


do not depend on the volume by summing up (12) over all possible 


along with quantities which 


values of < (and taking into account that +r; =O) we get JN, the 
total number of systems in the ensemble. So we find 
) 2 
— Y all ae 3S ¢ oc 
e O— _—_ wy Vn 929 4 
VA 


the quantity A being the discriminant of the quadratic form in the 
exponent. 


When we write 2,9,; =a, we find for the pressure p= — — 


53 
Proceedings Royal Acad. Amsterdam. Vol. XVII. 


800 


9 


Den dlgw aw 
SS SP i SS 
7) J dy 


A—s being very small with respect to the other factors, we may 


20. V? 


neglect its influence in w?'). The equation of state has the same 
form as vAN perk WaAALs’ equation. However, the correlation is sensible 
in the accidental deviation; for it changes the value of 17; and 
rt, which vanish if the correlation is neglected, obtain values 
deviating from zero. 

Denoting by A. and by 4,. the minors of the discriminant, 


we have 


= = (k—1) 


“ 7,02 = — (k—1) ’) 
A 
where J is the number of elements into which the volume is divided. 
as if Res tea Oe) E 
rhe condition &4 =O is equivalent to the condition = 0; For 
au 
if we write down the determinant in some arrangement, and if we 
add all rows to the first row, we get a determinant of which all 
terms of the first row have the form 
l ld .dlgw 1 


| a = 
Y yp da da Odv 


NPs: 


Strictly speaking, this is not true for some terms at the end of the row, 
but as we have neglected the action on the borders, we may neglect 
this fact too. In reality our considerations are only true for an infini- 
tely great volume, where this difficulty disappears, as A is then an 
infinite determinant. 

Now if 

De eee 


— U = i= 
yp Y da Odv oe 
then Ay—10) 
OrmitAv=="() 
d _dfw a 
——a ~—+ —-a=0 
da da (0) 
i ; _, dp 
which therefore agrees with 5 = (i), 
dv 


1) Cf Le p. 129. 
2) Cf. Ornsvery, Accidental deviations in mixtures. These Proceedings 15, 
p. D4, (1912). 


801 


The quantities rr, ete. here found are related to those mentioned 
above. And though a statistical deduction of the function / enter- 
ing into details’ may lead to difficulties, yet it is clear that 
statistical mechanics yield a correlation analogous to that expressed 
in g. 

If we should wish to continue the deduction of the conditions of 
the critical point, we should have to use higher powers of r,, which 
can be done without difficulty; we then find for the second condition 
ee) 
de? 

If we drop the supposition that the sphere of attraction is large, 
we can use the function %, defined in the quoted dissertation. In 
order to take into account the correlation, we must suppose the 
integrals 

é Gh Pon oc dan Tt, w (n,) 


1 


r — &/0 


defining %, to depend on nz for the element in question and also 
on the numbers of molecules in the surrounding elements. Therefore, 
in general, the numbers of molecules of all elements will appear in 
: O9n, 
9n, , but the influence of distant elements is so small that —— 
Ne 
‘an be put zero. 
By considerations analogous to those used in the quoted disserta- 
tion, we can show that %(n,) has the form 
Ny Nx 
V, (@ dy Dy, Dy) 
in which n,n, denote the densities (molecular), in the elements 
with which V, is in mutual action. The values of all n, are equal 
for the most frequent system. 
Now we find for ¢ 
Ga nia (uns ny Ms ts eae 
where P is a quadratic form in the deviations for the various 
elements, containing squares as well as double products. The form 
might be easily indicated, but we will omit it, as it is only our 
purpose to show how in general the statistic-mechanical considera- 
tions, changed in the sense of a correlation of elements of volume, 
lead to formulae analogous to those given in § 2. Here too the 
mean square of deviation and the means of double products are 
represented by quotients of minors of the discriminant of P and 


eeu : the “Freee : 
this quantity itself. Here too for : =0( the discriminant vanishes. 


av 
53% 


802 


4. The above considerations can be applied in ealeulating the 
critical opaleseence. For that purpose we use the simple method 
indicated by Lorentz"), whieh consists in superposing the light- 
vectors caused by the intluenee of every individual molecule in a 
point at great distance. 

Consider in the substance through which a beam of light passes, 
a volume J” great with respect to the wave-length, and take a distant 
point P, the direction |7P forming an angle gy with the incident 
Tay. 

All molecules lying in one plane perpendicular to the line which 
Take therefore a 
system of axes with the Z-axis parallel to this line, then the con- 


bisects the angle y, will cause equal phase in 7. 


tribution of one molecule will be 


9 


_ Qa 
B sin — (ct + 22 cost gp) 
ud 


where p. depends only on the kind of molecules, on 4 and on the 
distance |’P, w being the index of refraction. 
The number of molecules in dv dy dz amounts to 
(a + v) dex dy dz. 


The total light-vector in P? thus becomes 


2 fe +r) sin = Ae +22 cos bq) da dy dz. 


: 
and the intensity 
pile 
» 
re _ 2a 
Bp? ell [J a-+ p;) (a +-v-) sin — (ct4-22, cos } gp) 
ud 
) are 


on 
sin 


\- 
~ 

sS 

~— 


dx; - dz, dv. dy- dz-. 


Integrating with resp. to /, we get 


. 4n } - 
ae: # {fie -a(v,+ py.) -| v.»-! cos a (2,—<-) cos 8 y } da, dy,dz,da,dy-dz.. 
uA 
VV 


The-mean value of this must be caleulated. The term with », +- v- 
vanishes, and that with a? yields no contribution proportional to V. 
We introduce the value of »,»- from formula (10), and for c=t 
from form. (9). This gives 


1) H. A. Lorentz, On the scattering of light by molecules, These Proceedings 13 
p. 92 (1910). 


803 


— ap : ay ie ) = ( =v ) i ] 
i = Yes Wr, a Yrs So ez SNe Sr) diigo + MY = 
ali av -{- Ee [fo (Ws Ury Y UE cos 0 7] 
VV 


For a great volume one integration over VV can be performed 


(compare the deduction of formula (41)); further we put aV=N 


. Ax 
and for the sake of brevity —cos}gy=C, then we get 


{ur 
Ps 
1 — ws ye 
ue Als J feos Cz (#, y, 2) dadydz 5 oie 4(t8)) 


The integral appearing here will be represented by G,, that of 
formula (11) by G. It will be seen that the deductions criticised in 
§ 1 yield an opalescence proportional to v*,a quantity which accord- 
ing to the above is proportional to i + G, whereas the opalescence 
is proportional to 1+ G. 

With the aid of the integral-equation (6) we can express G and 
(, in the corresponding integrals of the funetion f. which we will 
indicate by / and F.. 


Integrating (6) with ah to xyz eat —o to + om, we find 
= 
[J fo wyz) da ty de (fos smi ffi + §,y +-3),2 +$) dudyde= 
de 
ne 
{ffi ‘(ayz) dndydz 
or i 
ean At eh od 
1—F 
Multiplying (6) by cos Cz and again integrating, we get 
pa as al 
G. — SL (S75) azine f fosc (2+$) cos CO4- sin C (z +8) sin CS 


——@ 
F(@+§, y+n, 248) dedydz = F,. 
The integral with the sines disappears because / and g are even 
functions; we find 
F. 
(a ek ie |) 
1— Ff, 
In order to apply the results obtained and to test them experi- 
mentally, one might try to deduce f from molecular theory. This 
would at best be possible under very simplifying suppositions and 


S04 


even then only an approximation can be obtained. Therefore we 
will take another way. As remarked in § 1, the exact value of x? 
for very great volumes was already known. In our notation we have 


=) TEP ae 
; cio aN dp 
yeas 

dv 


where .V is the number of AvoGrapo, v the molecular volume. 
According to formula (4) we have 


In the critical point = 1. ') 
The formula of opalescence first arrived at by Kresom and Ensrern 


1) There appears to exist a closer correspondence between the given statistic- 
mechanical method and the method using general considerations of probability, than 
perhaps might be expected. The elements of the discriminant (which is an infinite 
determinant in the former) agree with the function f in the latter. The former finds 
from this the value of ¥- vz as the quotient of a minor with that discriminant, 
the latter deduces this value from an integral-equation. In the critical point the 
discriminant vanishes, corresponding to this the FrepHotm determinant of the 
integral-equation is likewise zero. Thal this is the case when /’=1, appears by 
more closely studying the equation 


a (Sys) — i fo (S76) f (@-+8, y+, -+$) d§dnd§ = 0 


which only permits appropriate solutions if 1= >, (i e. this is the only proper 


I 
value). For /=1 this is therefore the case with the equation (6) without second 
member. 
From the formula (15) it will be seen that form. (6) can be solved by aFourtER 
integral. Putting 


+a 
l| {eo ma cos ny cos lz f (wyz) dadydz = —p (m, n, 1) 
afte 
—o 
we have ‘ 
+a 
1 “CC pm, n, 2) 
g (ayz) = ———— cos mw cos ny cos lz dmdndl. 
82° JIT 1—e(m, n, 1) 
wo 


805 


(#) 
ee | = 
Top, 22°V RIT dv 
Ope ie Aioast eee berate. 5s 2, (16) 


BE DPR Pa 


in which represent 
PD distance of observation 
mw index of refraction, 
y angle of electric force in ineident light with direction of 
observation, 
will likewise be found by using in (13) the value found for instead 
of #.. The exact formula then will result by multiplying by 


2 2) 


* f(ayz) dedydz. 


bass 

| 

yy 

|| 
ro} Q 
23 


Representing this integral by « and introducing the value of C, 
we get 
7 7 2 é % 
F— F.= 4n’ (1 + cose) { —}). 
te 
The formula of opalescence then will be: 


Top. ID Iss dv 
= = BS aed enol KC) 
i dp RI El\a 
— — + 4n*? — (1 + cos) 
dv vy a2 
In the critical point itself it therefore is 
1 2 
ONS ae ere w 
Lop. J dv 
—— eG eee lee age Oe) 


IT Dt Ne (t + cos) 


The greater exactness of form. (17) as compared with (16) is 
5 

confirmed by the measurements of one of us (Z.). According to these 

measurements, which however bear upon a mixture of liquids the 


1) According to this formula the proportionality of the opalescence to d~4, 
which holds for higher temperatures, changes continuously in the immediate 
neigbourhood of the critical point, into proportionality with %—2. This rea/ “getting 
whiter” of the opalescence should not be confused with the appurent changing of 
colour which is always observed much farther from the eritical point. The latter 
indeed is only a result of the method of observation, as is clearly proved by the 
measurements of one of us (cf. ZuRNIKE thesis). 


806 


reciprocal value of a quantity proportional to the opalescence changes 
linearly witb the difference of temperature 7’—7;, but by extrapolation 
does “not vanish for 27. “but for 777 — 10.0125 aWihen 
therefore for this value of 7—TZ;, the denominator of (17) is equal 
to zero, we can find from this, using VAN DER Waats’ equation, an 
estimation for ¢/,. The calculation yields : 


€ A » 
= = 00,0022 or ¢ = 1,2.10—* em. 


The quantity «is a measure for the size of the sphere of attraction. For 


+x 
1 
— Affe T (eyz) dadydz 
o - 


(go distance to origin) whereas in the critical point 
of 


{ F (wyz) da dy dz=1. 


ve} 
If f were constant within a sphere with radius R, then «* would 
be */, R?, and the above estimation would give 


el Omercits 


SUMMARY. 

1. The known formulae of critical opalescence give an infinite 
value at the critical point. Efforts to escape from this difficulty have 
furnished formulae for the deviations of density with a dependence 
upon the volume, at variance with the assumed mutual independence 
of the elements of volume. 

2. In order, to obtain formulae applicable in the critical point, it 
is found necessary to take into account the mutual influence of the 
elements of volume, it being shown that near the critical point this 
influence is sensible for distances large in comparison with the radius 
of the sphere of attraction. 

3. Two functions are introduced, one relating to the direct inter- 
action of molecules, the other to the mutual influence of two elements 
of volume. An integral equation gives the relation between the two 
functions. 

4. Corrected values are found for the mean deviations, and in 
the formula of opalescence a correction is introduced. The latter 
depends upon the sphere of attraction which can thus be calculated 
from observations. 

5. Further it is shown that the same results may be arrived at 
by taking into account the mutual influence of the elements of 
volume in the deductions of statistical mechanics, 

Groningen, Sept. 1914. 


A. A HIJMANS VAN DEN BERGH and J. J. DE LA FONTAINE SCHLUITER. ,, The identification of 
traces of bilirubin in albuminous fluids.” 


Bilirubin from human ascites fluid 3ilirubin from human ascites fluid 
(Aether-method) (Chloroform-method) 


Proceedings Roval Acad. Amsterdam, Vol. XVII. 


807 


Physiology. -- “Zhe identification of traces of bilirubin in albu- 
minous fluids.” By Prof. A. A. Hismans vaAN bEN BrrGu 
and J. J. pe ua Fontaine Scuiurrer. (Communicated by 
Prof. H. J. Hampureer). 


Several investigators have tried to demonstrate the presence of 
slight quantities of bilirubin in albuminous substances, for instance 
in normal human bloodserum. Most of them did this by adding 
various oxidizing substances, either directly to the serum or to an 
alcoholic extract of the latter. The first oxidation-stages of bilirubin 
having a green or a blue colour, the presence of bilirubin was 
regarded as established if an addition of these oxidizing substances 
eave rise to a green or a blue colour (OpeRMAER and Popper, STEIGER, 
Gitpert') and others). AvucnHé*) employed a much more reliable 
method based on the fact that bilirubin, in alkalic solution in the 
presence of oxide of zine, is changed, by careful oxidation with 
iodine, into a substance with a characteristic spectrum. This reaction 
had already been deseribed by Sroxvis, but Avcné, who mentions 
Sroxvis’ work, owns the merit of having stated accurately the con- 
ditions required if the reaction is to take place with absolute cer- 
tainty, so that it may be used to demonstrate the presence of bilirubin. 

Undoubtedly the reaction of Sroxvis-AucHE can be used with success. 
Only the spectrum-line is very slight in the case of the small amounts 
of bilirubin dealt with in this treatise: if the presence of bilirubin 
is to be demonstrated in normal human serum by means of this 
method, the layer of fluid intended for spectroscopic investigation is 
to have a thickness of ten centimetres. And even then the result is 
not always a positive one. For quantitative determinations this method 
cannot be used. 

Bieri extracted the serum at once with chloroform and carried 
out his reactions with this *). 

The reaction of Enrucn has supplied us with an excellent means 
of tracing bilirubin in bloodserum and other albuminous fluids and 
of determining it quantitatively ‘). The characteristic difference in 
colour between av alkaline and an acid medium increases its relia- 
bility, whilst the reaction is an extremely sensitive one. It must, 

1) OBerMAWER u. Pepper. Wiener Klin. Wochenschr. 1908. 

Sreicer. Dissert. Ztirich 1911. 

Gitpert. See for his werks the bibliography in: Clinique médicale 1910/1911. 

2) Aucueé. Compt. rend. Acad. d. Sciences 108. 

3) Bieri. Folia Haematolog. 1906 ILI. 189. 

') Hismans van pEN Berg and Snapper. Deutsch. Arch, f. klin. Med. 1913, 


808 


however, be admitted that neither this nor any other colour-reaction 
enables us to identify the presence of bilirubin with absolute certainty. 
The possibility of other substances contained in the serum giving 
the same reaction with the diazo-body may be esteemed less probable, 
it cannot with absolute certainty be denied. 

As far as we know it has hitherto been found impossible to 
isolate bilirnbin from normal human serum, which would have 
afforded an incontestable proof of its presence. HAMMERSTEN has 
attempted it’). But though in a great majority of cases he obtained 
fine bilirubin-erystals from horse-serum, he never succeeded in ob- 
taining them from normal human serum. From the terms used in 
the latest edition of his Handbook of Physiological Chemistry we 
eather that this investigator is not quite convinced yet of the presence 
of biluribin in normal human serum. 

With a view to researches on anhepatic bilirubin-formation we 
needed a method which would enable us to identify with absolute 
certainty the presence of small quantities of bilirubin in bloodserum, 
exsudates and transsudates, if possible by obtaining the pigment in 
the form of erystals. After some experiments we have succeeded in 


this, starting from the property of bilirubin — which we have not 
found mentioned anywhere — of dissolving readily in acetone. 


To 10 em*. of bloodserum 20 em’. of pure colourless acetone are 
added. An albumen precipitate is formed, which is centrifugalized. 
The fluid at the top, coloured more or less intensely yellow, contains 
all the bilirubin and only traces of albumen. This liquid is evaporated 
in vacuo at the ordinary laboratory temperature. 

If one has a good vacuum-pump at one’s disposal the liquid soon 
begins to boil; after some minutes the acetone is evaporated. A watery 
fluid remains in which, besides other serum-substances, all the bili- 
rubin is dissolved. Then the fluid is shaken 2 times or more with 
aether to remove the fatty bodies as much as possible. 

These pass into the aether which is pipetted. The last traces of 
aether are removed in vacuo. The aether may of course also be 
removed by means of a separatory. Then a certain amount of chloro- 
form e.g. 2 em*. are added, the fluid is slightly acidified with HCl 
and shaken. The bilirubin then passes into the chloroform. By centri- 
fugalization the watery fluid can easily be separated from the chloro- 
form. The chloroform is washed thoroughly with water to get rid of 
all the hydrochloric acid and centrifugalized onve more, the water being 
removed by means of a separatory or by pipetting. Traces of water, 
however, remain mixed with the chloroform, which sometimes renders 
; 1) Hanmarsren, Maly’s Jahresber. 1878 Il. 119. 


809 


the fluid slightly troubled. These traces of water are removed by 
shaking with glowed sulphate of sodium. The latter is removed by 
filtration. The result is a very pure solution of the yellow pigment 
in chloroform (solution A). It may be easily proved that this yellow 
pigment is bilirubin. 

1. If the chloroform solution is shaken with diluted KOH or NaOH 
the pigment passes into the latter, while the chloroform loses its 
colour (solution £). 

2. If now some acid is added till the fluid reacts distinctly as an 
acid, then the fluid at the top loses its colour, the pigment passing 
into the chloroform at the bottom. 

3. If to the alkaline solution (see sub 1) HNO, containing some 
HNO, is added, the result is the well-known colour-play of the reaction 
of GMELIN. 

4. If a slight quantity of a diluted iodine-solution in alcohol 
(1: 100) is carefully poured on to the alkaline solution, a blue ring 
is formed. 

5. If to the alkaline solution first an equal volume of alcohol is 
added, and then +} of the original volume of the diazo-mixture ot 
Enriuicu, a red colour is the result. An addition of a few drops of 
concentrated HCl changes the red colour into blue. 

_All these reactions together, prove conclusively that the pigment 
obtained in the above way is indeed bilirubin. 

Crystals of bilirubin can be easily obtained from the pure chloro- 
form-solution (sol. A) in the following manner. The latter is poured 
ont into a wateh-glass which is covered with another watch-glass 
and placed in the ice-safe. The chloroform evaporates slowly and 
on the watch-glass the microscopically visible, pretty, yellow bilirubin- 
crystals are left. When HNO, containing HNO, is added, these 
crystals present under the microscope the reaction of Gmrnin. 

We can also dissolve the yellow crystals again in some solvent 
(chloroform, dil. NaOH ete.) and carry out the above-mentioned 
reaction with them. 

If one has no good vacuum-pump at one’s disposal the method 
ean also be applied with the following modification suggested by 
Dr. SNAPPER. 

10 em* of bloodserum are precipitated with 20 em* of acetone. 
The albumen-precipitate is centrifugalized. To the pipetted upper- 
fluid some drops of water are added; then this fluid is washed 
carefully with aether a few times, to remove the fatty substances 
as much as possible. These volumes of aether are removed with 
the pipette every time. Then some drops of ice-vinegar and 1 em* 


810 


of aether are added to the fluid. All the bilirubin passes into the 
mixture of ice-vinegar and aether, which separates entirely from 
the fluid underneath. If this yellow-coloured aether is pipetted and 
placed in an ice-safe in a loosely covered watch-glass, we likewise 
observe that crystals are formed. 

The accompanying ~ picture is a micro-photograph of bilirubin 
crystals which we obtained from the ascites-fluid of a heart-patient, 
and from normal human serum. 

Attempts to produce bilirubin-crystals by the above-mentioned 
method from the intensely yellow-coloured serum of two icterus- 
patients, led to a remarkable experience. If namely we placed the 
chloroform-solution which, as appeared from various reactions, con- 
tained much bilirubin, in the ice-safe, for the purpose of a slow 
evaporation, the yellow colour at a certain moment when, owing to 
the evaporation of the solvent the concentration had reached a certain 
value, suddenly passed over into a green one, evidently by a change 
of the bilirubin into biliverdin. The same phenomenon occurred 
when we evaporated the chloroform-solution in vacuo. It must be 
distinctly understood that this occurred only with the solution obtained 
from the serum of patients suffering from obstructive jaundice. We 
cannot give an explanation of this phenomenon. Most likely the 
icterus-serum contains substances promoting the oxidation of bilirubin 
into biliverdin. 


Botany. — “Gummosis in the fruit of the Almond and the Peachal- 
mond as a ‘process of normal life.” By Prof. M. W. BrisErinck. 


(Communicated in the meeting of September 26, 1914). 


[t has hitherto been generally accepted that the formation of gum 
in the branches of the Amygdalaceae always is a process of patho- 
logical nature. I have found that this opinion is erroneous, and that 
gummosis occurs normally in the fruits of the Almond (Amygdalus 
communis) and the Peachalmond ( Amygdalus amygdalo-persica ) 
DunameL Dumoncrav. *) 

1) In some Dutch nurseries the peachalmond is simply called *Almondtree”. 
The difference is in fact very slight as it consists only in the drying up of the 
almond fruit before the epicarp opens, and the position of the flowers in pairs, 
whereas the fruit of the peachalmond remains fleshy even at the dehiscence, and 
its flowers are mostly single. Between leaves, flowers and branches no con- 
stant differences are found. 

GRENIER et GopRon (Flore de France T, 1, Pag. 512, 1848) call the peach- 


S11 


Contrary to what might be expected the phenomenon is the more 
obvious as the trees are better fed and more vigorous. In specimens 
on sandy grounds it can only be observed with the microscope. 

As gummosis is the effect of a wound stimulus, if is of import- 
ance that this process also takes place in the normal development 
of the healthy plant. The subject is moreover of practical interest. 
All the chief facts relating to gum formation can almost unchanged 
be apphed to the production of gums in general, of gum resins, 
and of resins, among which are substances of great medical and 
technical value. As the study of the influence of parasitism has made 
it possible to produce gum, and no doubt many of the other sub- 
stances mentioned, in a more rational way than has been done till 
now, a short review of the whole subject seems not superfluous. 


Wound stimulus as cause of gummosis. Poisoning, and 
parasitism also causes of this stimulus. 


Gummosis in the Amygdalaceae is a process of cytolysis, whereby 
young cells, freshly sprung from cambium or procambium, and 
sometimes also young parenchyma, are more or less completely 
dissolved ‘and converted into canals or intercellular spaces, filled 
with gum. In dissolved parenchymatous tissues usually remains of 
not wholly disappeared cell walls are found; the gum of the phloem 
bundles is more homogeneous, but always the microsomes of the 
dissolved protoplasm are found. The nitrogen of the gum springs 
from the dissolved protoplasm. 

Formerly we proved’) that by such different causes as poisoning, 
parasitism and mechanical wounding gummosis may be experimentally 


almond Amygdalus communis var. amygdalo-persica. At present the name 
Amygdalus persicoides (Koon, SERINGE, ZABEL) is also used, as in the Hortus 
of the University of Leiden. The opinion that it is a hybrid is not sufficiently 
founded. When grown from seed the tree seems constant (see Mreter’s Conver- 
sationslexikon, Articles “Mandel’’ Bd. 11, p. 853 and “Pfirsich” Bd. 13, p. 782, 1896) 
and identic with the “English almond”, of which Darwin reproduces a stone 
(Domestication, 2nd Ed., Vol. 1, p. 858, 1875). The fruit is fleshy and bursts 
open, the kernel is edible, not bitter. At Delft sowing experiments have been 
going on a long time already, but under unfavourable circumstances. The root 
cannot resist the winter temperature of the soil, hence, grafting on the plumtree 
is required. 

1) M. W. Bevertnck et A. Rant. Excitation par traumatisme et parasitisme, et 
écoulement gommeux chez les Amygdalées. Archives Néerlandaises, Sér. 2, T. Il, 
Pag. 184, 1905. — Centralblatt f. Bakteriologie, 2te Abt., Bd. 15, Pag. 366, 
1905. — A. Rant: De Gummosis der Amygdalaceae. Disserltatie Amsterdam, 
Bussy, 1906. 


provoked in many Amygdalaceae, as almond, peachalmond, apricot, 
peach, plum, cherry, and bird’s cherry. 

But these three groups of causes may all be considered from one 
single point of view, by accepting that gummosis is always the effect 
of a wound sumulus, proceeding from the slowly dying cells, which 
are found as well in every wound, as at poisoning and parasitism. 
These dying cells may change into gum themselves, but besides, exert 
their influence on cambium tissues to distances of some centimeters. 
This distance-influence is the principal effect of the wound stimulus. 
But poisoning by sublimate or oxalic acid, introduced under the bark, 
can as well excite gummosis as an incision or a wound by burning 
or pricking. Neither the dead cells nor the poison are the active 
factors here; the stimulus proceeds from the slowly extinguishing cells, 
so that gummosis is essentially a necrobiotic process. Probably the 
dying cells, after the death of the protoplasm, give off an enzyme 
or enzyme-like substance, a lysine, fixed during active life, but, which 
being freed by necrobiosis and absorbed by the young division produets 
of the cambium causes their cytolysis. This reminds of the eytolysimes 
of the animal body, originating when foreign cells are introduced, 
which liquefy the corresponding cells, for example the haemolysines 
which dissolve the red blood-cells. Furthermore of the bacteriolysines 
and of cytase, the enzyme of celiulose. 

If the hypothesis of the existence of a “gumlysine” is right, — and 
I think it is, — this substance must be of a very labile nature, for 
when bark wounds are infected with gum, quite free from germs 
of parasites, no more abundant gummosis is observed than at 
mechanical wounding only. But a difference, however slight, will 
certainly exist. 


Gummosis produced by wound stimulus. 


The influence of this cause is best studied in the following experiment. 

A deep wound, penetrating into the cambium of a branch of 
almond or peach, commonly soon heals completely, but it may be 
that gum flows from the wound. This is the case when the trees 
are in sap, thus in February or March at temperatures above 20° C. 
and below 33° C. The experiment succeeds best with cut branches 
in the laboratory. When the wounds are made in the open air in that 
season no gummosis ensues, the temperature then being too low.) In 


1) If the wounds are infected with Corynewm, an extremely copious gum production 
follows in spring, as the parasite then finds abundant food in the branches. There 
is, however, no season when wounds, infected with Corynewm, do not sooner or 
later yield gum. 


813 


summer the cambium of the still longitudinally growing part of 
young green branches may be caused to form gum by punctures or 
incisions, but these wounds heal quickly, except when ‘kept open” 
by Coryneum or other parasites. 

As to thicker branches, wounded in spring, the microscope shows 
the following. 

Around the wound a great number of gum canals are formed in 
the cambium, about parallel with the axis of the branch, some centi- 
meters long, which become the thinner and shorter as they are 
more remote from the wound. The canals are separated by the 
medullary rays, which are with more difficulty converted into gum than 
the phloeoterma. All the gum canals together form a kind of net- 
work, whose meshes are filled by the medullary rays. The whole 
network has the shape of an ellipse, the “gum ellipse’, the wound 
lies in the lower focus towards the base of the branch. The stimulus 
extends over the ellipse, evidently farthest in the direction of the 
branch, less far towards the base and sideways. So it may also be 
said that the wound stimulus extends farthest opposite to the “de- 
scending” current of nutrient inatter, following the phloem bundles, 
or along with the “ascending” water-current, following the wood. 
Evidently the gum canals are more easily formed in the better fed 
ceils above the wound than in those beneath it, where the nutrition 
must be worse. This is especially obvious in ringed branches. Wounds 
in the cambinm, directly above the ring produce much more gum 
than those immediately below. ’) 

Under ordinary circumstances the branches, after simple mechanical 
wounding, are soon completely healed, and if the cambium at the 
outside of the gum canals then again begins to produce normal 
secondary wood, the gum canals may later be found back in the 
wood itself.*) Evidently the healing takes place as soon as the 
stimulus ceases, and so it is not strange that when it continues 
by poisons or parasitism the gum production also continues. 


1) The nature of the power, by which the food transmitting, ‘“descending” 
sap current moves through the phloem bundles, is not known, It is thus not 
impossible, that if the cause of gummosis is of a material nature, a lysine, moving 
through the tissues, it is able to run in opposition to the ‘descending’ current. 
I think, however, that the extension of the stimulus does not go along the phloem 


but along the xylem bundles and the young wood, with the “ascending” sap. 


2) [ have never seen distinct gum canals in the secondary wood, but according 


to the descriptions they occur eventually. 


sl4 


Parasitism as cause of guinmosis. 
The connection between wounding and parasitism. 


Wounds in peach branches treated with poisonous substances, 
such as sublimate, produce gum much longer and more copiously 
than the like wounds without sublimate. Other poisons have quite 
the ‘same effect. Now it is clear that the direct intluence of para- 
sitism on the organism must be sought in the action of some 
poisonous substance. Hence it seems ceriain that what these three 
causes have in common, namely necrobiose, or the slowly dying of 
the cells surrounding the dead ones, is the base of gummosis, and 
that parasitism, where necrobiose lasts as it were endlessly, must 
be the most powerful instigator of the process. 

That this simple view of the question has not yet taken root in 
science is proved by the most recent treatise on our subject by 
Mikoscu,') illustrated) with beautiful anatomical figures. After the 
publication of Dr. A. Rant and myself of 1905, he described the 
relation of mechanical wounding to gummosis. But he did not think 
of poisoning experiments, nor has he any belief in the influence of 
parasitism on gum formation. Wisner, in his recently published 
paper on gums in the new edition of his ‘“Rohstoffe des Pflanzen 
reichs’, is also of the same opinion as Mixoson. 

For my. object a short discussion of a few examples of parasitism 
will suffice. 

The little caterpillar Grapholitha weberiana makes borings into the 
bark of plum and apricot, and if the outermost corklayer is removed 
by shaving it off, the butterfly finds so many fit places for deposing 
its eggs, that the larvae creep in by hundreds and make new borings 
from which later the gum flows out. These holes are coated with 
a layer of slowly dying cells, whence the stimulus extends, which 
produces the gum canals in the contiguous “cambium”. By cambium 
I simply understand the not yet differentiated division products, 
“young wood” and young phloeoterma. The necrobiotic cells, clothing 
the continually extending holes in the bark, and the great numbers 
of new individuals of the caterpillars, make the gum production a 
chronical process. 

To explain the formation of the enormous quantities of gum 
produced in this way, it seems only necessary to think of mechanical 
wounding and not of any special excretion from the animal. But it 
must be noted that the space, where the caterpillar lives during its 


1) Untersuchungen tiber die Entstehung des Kirschgummi. Sitzungsber. d. Kais. 
Akad. d. Wiss. in Wien. Mathem. naturw. Klasse. Bd. 115, Abt. 1. Pag. 912, 1906. 


S15 


erowth, namely a vertical narrow canal in the inherbark, very near 
to the cambium, could not possibly be imitated artificially. 


a 


Fig. 1. (Natural size). Gum producing peachalmond in September, whose 
summit is cut off; the gum from the gum canals is afler drying, swollen by 
moistening with cold water. 


Much more common and interesting than the animal parasites are 
the gum producing Fungi of the Amygdalaceae, five of which are 


found in our country.') The commonest and most vigorous is Cor- 


1) Coryneum beyerinckii OupEMANS, Cytospora leucosioma Prrsoon, Monilia 
cinerea BonorDEN, Monilia fructigena BoNnoRDEN and Botrytis cinerea PERSOON 
(see Rant, l.c. p. 88). German authors also mention bacteria as instigators of 
cummosis, | never found them. 

a4 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


SI6 


yneum bejerinckii Ouvemans (Clasterosporium carpophilum Apgru.).") 

Pure cultures of Corynewn in bark wounds of almond, peachal- 
mond, peach, cherry, plum, bird’s cherry, sloe, virginian plum, develop 
with remarkable quickness and soon make the bark die off, evidently 
in consequence of the secretion of a poison. Around the dead cells 
ihe necrobiotie are found from which the stimulus issues, which, 
penetrating into the cambfum .in the usual way, forms gum 
canals in the young wood. Many mycelial threads of the parasite 
itself are then cytolised and converted into gum. I think this facet 
remarkable and a strong argument for the material nature of the 
stimulus. 

Undamaged branches are with difficulty infected by the parasite, but 
it is easy, even by very slight wounds and artificial infection, if — 
only the wounds be numerons, to obtain great quantities of gum. 
This circumstance explains why nursery men dread wounds in the 
trunks and branches of stone-fruit trees. 

In the green shoots, especially of the peach, the formation of 
anthocyan is observed in’ the enfeebled tissue around the wounds 
infected with Corynewim when exposed to sunlight. *) 

The supposition that secretion products of the parasitic caterpillar 
or the Fungus could be the direct cause of the stimulus, is contrary 
to the positively existing relation between mechanical wounding and 
o1UNMOSIS. 


Gum canals in the fruitilesh of almond and peachalnond. 


To the preceding facts, long since stated, I wish to add the following. 
Already in my first paper of 1883 I called attention to the cireum- 
1) BetERINCK, Onderzoekingen over de besmettelykheid der gomziekte bi planten. 
Versl. d. Akad. v. Wetensch. Amsterdam, 1883. — Contagiosité de la maladie de 
gomme chez les plantes. Archives Néerlandaises, 1é Sér., T. 19, Pag. 1, 1886, — 
Cc. A. J. A. OupEMANS, Hedwigia, 1883, N°. 8. — Saccarpo, Sylloge Fungorum, 
Vol. 3, Pag. 774, 1884. — AprERHOoLD, Ueber Clasterosporium carpophilwm (LEy.) 
ADERH. und dessen Beziéhung zum Gummifluss des Steinobstes. Arbeiten der 
Biolog. Abt. am Gesundheitsamte zu Berlin. Bd. 2, Pag. 515, 1902. ADERHOLD 
has experimented with pure cultures of Corynewm, which | had made and sent 
him. He himself has not executed any isolations of gum parasites. His determination 
as Clasterosporium amygdalearum (L&y.) is thus founded on the imperfect de- 
scriptions from the older mycological literature, in which OupEMANS was no doubt 
better at home than he. Like Linpau [ reckon Clasterosporiwm to another family 
than Coryneum. 

2) The apperance of anthocyan in the light is commonly a token of diminished 
vitality and often a consequence of necrobiose in the adjoining cells. Hence, wounds, 
poisons and parasitism cause anthoeyan production in the most different plants. 


817 


stance, that in the fruit-flesh of the peachalmond, and as I may add 
now, also in that of the almond itself, there is a system of gum 
canals, precisely corresponding to that of the vaseular bundles. Of 
these the phloem bundles are converted into gum canals by cytolysis, 
either entirely or with the exception of the outer protophloem ; the gum 
canal (gp Fig. 2 and 3) thus, is always immediately contiguous to 
the woody bundle 2d. 


Fig. 2 (38). Gum canals in the transverse 

section of the fruit-flesh of a peachalmond : 

ha. hairs on epidermis ; 20 dermoidal tissue; 

bp chlorophyll-parenchyma; #/ xylem bund- 

les; ph phloem bundles; gp gum canals 
sprung from phloem bundles. 

Fig. 2 and 3 are reproductions from my 


above mentioned treatises of 1883 and 1886. 


The presence of gum in the canals of the fruit is easily shown. 
In August or September the summit of a peachalmond fruit is cut 
off and the fruit, or the branch with the fruit, is placed in water. 
After some moments all over the section droplets of gum are seen 
evidently issuing from the vascular bundles. As these bundles 
are distributed through the fruit-flesh, running longitudinally and 
transversely, and are partly reticulated, the number of droplets is 
very great and they are of different size. In particular near the stone 
they are big. If in August the gum is allowed to flow out in cold 
water it dissolves completely or nearly so. In September the dissolving 
is nO more complete. By drying the gum, its solubility in cold 
water gets almost lost, but it continues in hot water. 

From lateral incisions also much gum flows out. In Fig. 1 the 
drops are represented after drying, followed by swelling up in cold 
water. 

Although this gum does not only consist of dissolved wall material 

54* 


$18 


but also of cell contents, the microscope can only detect fine granules, 
evidently corresponding to the microsomes of the protoplasm, which 
are not dissolved during the eytolysis [ could) not find back the 
cell nuclei in the gum, but in the cells of the not yet cytolised 
phloem bundles, they are neither perceptible. As under normal cir- 
cumstances the gum does not flow out, ifs volume must be about 
as great as that of the phloem bundles which are cytolised. It is, 
however, certain that the capability of the gum to swell up by 
imbibition is much greater than that of the cell-tissue which gave 
rise to its formation. It seems thus certain that imbibition with 


Nie 


Fig. 3 (360). Gum eanal with surrounding ; 
gp gum; x/ xylum bundles, unchanged; ph non- 
dissolved cells of the phloem bundles; cd thread- 
shaped cells in a gum canal, originating from the 
phloem bundles. 


sufficient access of water must lead to a perceptible pressure and 
also. some thickening of the fruit-wall. This must promote the 
opening of the fruit as well as the remarkable detaching of the 
stone, although the required mechanical power for these processes 
must, no doubt, chiefly be the tension of the tissue of the paren- 
chyma of the fruit-wall existing independently of the gummosis. 
Finally the stone is found quite loose within the fleshy shell, which 
mostly opens like a bivalvate mollusk, but sometimes shows three 
or four fractures. The vascular bundles, which pass from the fruit- 
flesh into the stone, are thereby torn off clear from the stone. At 
the base the separation seems provided for by an intercepting layer, 
as at the fall of leaves. 


819 


The portion of the phloem bundles within the stone of the peachal- 
mond is never converted into gum; in the almond itself such gum 
is found in rare cases inside the shell. 


Wound gun in the fruit-wall as a consequence of mechanical 
stress of the tissue. Gumming almonds. 


In many cases real wound gum is found in the fruits of the 
almond and the peachalmond, not proceeding from the gum canals 
but from fractures in the parenchyma of the fruit-flesh. Its origin 
must undoubtedly be sought in the tension or stress of the tissue, 
which causes the opening of the fruit. An additional circumstance, 
however, is required, namely a loss of vital strength, by which the 
regenerative power of the tissue that coats the fracture is annihilated. 
The therefrom resulting incapability of regeneration is associated 
with the ripening of the fruit in a way not yet explained and 
should rather be attributed to superfluous than to poor nutrition. 
Parasitism is wholly absent in the production of wound gum from 
the parenchyma of the fruit. 

The fracture is mostly at the side where the two edges of the 
carpels are grown together and the fruit later opens. Not seldom 
in this case is wound gum seen to flow spontaneously from the 
base of the fruit along the short peduncle. In other cases the wound 
is at the side of the middle nerve of the carpel. Always the edges 
of the fracture are coated with cells in a condition of necrobiose, 
which is evident by their quickly colouring brown at the air, which 
normal living cells do not. These necrobiotic cells and the adjoining 
tissue produce gum. With the microscope not quite dissolved cell- 
walls may be found in the gum, showing that the cells were about 
full-grown when the process began. 

In common almonds gum is sometimes found within the hard 
shell,') and eventually part of the kernel itself is then also changed 
into real wound gum with still recognisable remains of the cell- 
wall. In such almonds the phloem of the vascular bundles, whieh 
run through the stone to the funiculus, is always changed into a 
eum canal, so that the gum can reach the surface of the young 
seed. 

If we suppose that gummosis originates by the action of a cytolvsine, 
if seems very well possible, that the lysine which has flowed inward 
together with the ‘canal gum’, is able to attack the developing 
1) The small quantity of gum found, especially in “hard almonds”, at the 
surface of the shell, proceeds from the gum canals of the fruitflesh. The sugar 
Jayer which covers the shell of the ‘soft’ species is dextrose. 


820 


seed and is yet too labile to be demonstrated by infection of bark 
wounds with gum. Experiments in this direction may perhaps be 
effected with the peachalmond. 


Wound stimulus as factor of development. 

Formerly I thought that the presence of gum canals in the fruits 
was accidental and should be explained by parasitism, although I 
could not find any parasites. 

In later years, with better knowledge, 1 again examined the gum 
canals in the peachalmond and their surroundings repeatedly. Never 
did I find a fruit without them, but they were not equally developed 
in different trees from different gardens. In specimens of sandy 
grounds they can sometimes only be found with the microscope. 
Neither mucroscopically nor by experiments has it been possible 
to detect gum parasites. This makes it quite certain that in the 
formation of gum eanals parasitism is excluded. *) 

The great ease wherewith mechanical tension causes wounds in 
the fruit-flesh of the peachalmond, gives rise to the supposition, that 
the normal gum canals may be the product of some hidden wound 
stimulus. 

If this supposition is true, ave cannot think of wounding in 
the common sense of the word. When the flowers fall off, a 
ring-shaped wound forms around the base of the young fruit, 
but this is a normal process, taking place in an_ intercepting 
layer and soon followed by complete healing. In the flowers of 
peach, plum, apricot, cherry, we observe the same without any 
formation of gum canals in the fruit-flesh. Moreover, although the 
peculiar structure of the layer between the woody peduncle and 
the stone, along which the ripe fruit detaches, reminds of rent 
tissue, no gum is formed at that spot and the layer also exists in 
the other stone-fruits, where no gum canals occur. 

So long as nothing else has been proved it must therefore 
be accepted that in the phloem bundles of the fruit of the peachalmond, 
where cytolysis takes place, the same factor of development is active 
as that, which gives rise to the pathological gum canals in the cambium 
of the branches. This leads to the conclusion, that the wound stimulus 
belongs to the normal factors of development of this fruit, although 
nothing is seen of external wounds. When considering, that the 
phloem bundles are built up of extremely thin and _ soft-walled cells, 


') The supposition, sometimes met with in literature that the gum of the Amyg- 
dalaceae should consist of bacterial slime is quite erroneous. That parasitic bacteria 
eventually occur as gum parasites, as is stated by some authors, I do not think 
impossible, although till now I only found caterpillars and Fungi as active agents, 


821 


it is conceivable, that by great tension of the tissue in the surrounding 
parenchyma, they undergo strain and pressure causing mechanical 
rupture and necrobiose, centre and prey of the wound stimulus 
being the phloem bundles themselves. 

This conception is in accordance with the fact that the gum 
canals are broad in the fruits of well-fed trees on rich grounds, 
which have a hard and solid flesh, wherein stress and strain are 
certainly very great. Only here and there remains of the protophloem 
along the gum canals are still to be found in sueh fruits. But in the 
softer fruits of sandy soils, along the much narrower gum canals 
not only the protophloem is still present, but also stripes of the 
secondary phloem. 


Summarising we come to the following conclusions. 

Mechanical wounds in growing tissues of Amygdalaceae will some- 
times heal directly, sometimes after previous gummosis. 

The chief tissue, which is transformed into gum is the young 
secondary wood newly sprung from the cambium and not yet 
differentiated. By the wound stimulus a network of gum canals 
is formed around the wound. In thick branches, with a bark wound, 
this network has an elliptical circumference, the wound being in the 
lower focus of the ellipse, 

If the stimulus is removed by the cure of the wound, the cam- 
bium again continues to produce normal secondary wood, so that 
afterwards the gum canals may be found in the wood itself. 

If the stimulus continues the gum formation also becomes lasting. 

The stimulus issues from the cells that die slowly by wounding, 
poisoning or parasitism. Probably a cytolysine flows from these cells 
into the young wood or the procambium; these bind the lysine and 
liquefy to gum. Hence, gummosis is caused by necrobiose. 

Young medullary rays and phloembundles are with move difficulty 
converted into gum than the young secondary wood. But in the 
fruit-flesh of the almond and the peachalmond it is the phloem 
which changes into gum. The protophloem of the bundles often 
remains unchanged. 

Although gummosis in these fruits belongs to their normal develop- 
ment, a wound stimulus is nevertheless active. This stimulus springs 
from the strong tension in the parenchyma of the fruit-wall, which 
gives rise to tearing, necrobiose and gum formation in the delicate 
tissue of the phloem bundles. Consequently the wound stimulus is 
here a normal factor of development. 

It might also be said that the almond and the peachalmond are 
pathological species, but thereby nothing would be explained, 


822 


Chemistry. — “The allotropy of Lead.’ I. By Prof. Ernst Conen 
and W. D. Hinprrman. 
(Communicated in the meeting of Oct. 31, 1914.) 


1. Indications concerning the existence of allotropic forms of 
lead are found not only in the earlier chemical literature. Fourteen 
years ago Ernst Cowen’) pointed out in his studies on tin a clause 
in Piorarcr’s (50—120 A.D.) Symposiaca (VI, 8) in which allusion 
is made *) to the fact that lead is sometimes disintegrated spontaneously 
at low temperatures. 


This clause runs as follows: ‘No, the craving for food is not caused by the 
cold, but in the body something takes place similar to that which happens with 
metals in a very strong winter. There it is seen that cooling not only causes 
congealing, but also melting, for in strong winters CKOvEL o2(3dov (pieces of 
lead) occasionally melt away, consequently something similar may be supposed to 
take place in the intestinal process, elec... .” 

Moreover THESOPHRAST (390—286 B.C.) mentions such phenomena in his book 
aeQi AVQdS: “xatTitEQoY yo uci zat WoAUBdoy Ydy TaxFvae tv TO 
IIcvt adyou xa yEmoOrog drtog veavizot, yadxov dé Oayiva.” 
(It is told that tin and Jead melted sometimes in the Pontos when it was very 
cold in a strong winter, and that copper was disintegrated. 


2. Samre-Ciaire DevitLe*) stated that the density of lead is a 
function of its previous thermal history. He gives the following 
figures (water at 4° — 1; Temp. ?) 

After quick cooling of molten lead 11.363. 
er slow - * A ellen nae 

In a second experiment he found: 

Density of lead electrolytically deposited 11.542. 
After melting and rapid cooling 11.225. 

About the value 11.542 he says: 

“Mais telle est la rapidité avec laquelle se carbonate a l’air ce plomb extréme- 
ment diviseé, quil a fallu le transformer en sulfate pour en déduire ensuite le 
poids de la matiére employée. Cette complication introduil-elle quelque incertitude 
sur le premier nombre, ou ne doit on pas plutot ladmettre comme représentant 
la densité de ce plomb parfaitement cristallisé ?” 

3. These values as well as others given in earlier literature have 
to be aecepted with reserve as generally no data are given about 


1) Proceedings of the meeting of Jan. 26, 1901, p. 469. Zeitschr. f. physik. 
Chemie 36, 513 (1901). 

*) PLurarcut Chaeronensis varia scripta quae moralia vulgo yocantur. Lipsiae, 
ex officina Car. Tauchnitii 1820, Tomus IV, 339, 

5) ©. R. 40, 769 (1855), 


Prof. ERNST COHEN and W. D. HELDERMAN, ,,The Allotropy of Lead I”. 


(Natural size). 


Proceedings Royal Acad. Amsterdam, Vol. XVII. 


823 


the purity of the material experimented on and as there often 
exists some uncertainty concerning the method whereby the density 
has been determined. 

4. Kanipaum, Rotn and Siepier') found the density of a pure 


91° 


specimen of lead prepared by distillation in vacuo to be do 11.541. 


5. The values given by different authors for the specific heat of 
lead vary within wide limits, as may be seen from the table given 
in Arneae’s Handbuch der anorganischen Chemie.*) Moreover it may 
be called to mind that Le Verrier’) stated, that the specific heat 
of lead is a function of its previous thermal history. 

6. The facts mentioned above as well as the investigations of 
Storpa, *) and those of Orro LEHMANN *) render a new investigation 
of the subject very desirable. ‘ 

7. A year ago we carried out some experiments in this direction. 
As the results were negative we experimented with other metals, 
which yielded a more favourable result. Since a fresh investigation 
on lead has given positive results, as will be proved below, we 
give here also a short description of our earlier experiments, which 
taken together with the new experiments furnish a confirmation of 
the results obtained by us in the case of other metals (bismuth, cad- 
mium, copper, zinc, antimony). 

8. Our experiments have been carried out with lead which 
contained only 0.001 per cent of copper and 0.0006 per cent of 
iron (Blei-‘‘KaaLBAUM’-Berlin). °) 

The metal was turned into shavings on a lathe and washed with 
dilute nitric acid, water, alcohol and ether. After this it was dried 
in vacuo over sulphuric acid. 

9. The density of this material was found to be 


0 
P= de, 116398; 


b. 11.330, 


_ We put the, metal into an aqueous solution of PbCl, and kept it 
for 48 hours at 100°. After washing and drying it, we found: 


1) Zeitschr. f anorg. Chemie 29, 177 (1902). 
2) Bd. 3, 2te Abteilung, p. 633 (Leipzig 1909). 
3) Comp. Ernst Couen, Proceedings 17, 200 (1914). 
4) Journ. f. prakt. Chemie 94, 113 (1865); 96, 178 (1865). 
5) Zeitschrift f. Kristallographie und Mineralogie 17, 274 (1890). 
Ernst CoHen and Karsusr Inovyi, Zeitschr. f. physik. Chemie 74, 202 (1910), 
6) Mytius, Zeitschr. f. anorg. Chemie 74, 407 (1912), 


824 


d aa G5 1aES 297 
d. 11.328, 
Another part of the original material was melted and chilled in 
a mixture of alcohol and solid carbon dioxide. The determination 
of the density gave the following result : 
25° 


ioe 


e. 11.330, 
fF: dio33; 


10. As our determinations had been carried out with an accuracy 
of 3 or 4 units in the third decimal place, it is evident from the 
experiments described above that we had not been able to detect. 
any transformation in the lead experimented with. 

11. However, some months ago Mr. Hans Heuer at Leipzie was 
kind enough to call our attention to some phenomena which he 
described in the letter which follows : 


“Gelegentlich eines Vorlesungsyersuches, der einen sogenannten ‘Bleibaum” 
zur Darstellung bringen sollte, bereitete ich eine Lésung von 400 gr. Bleiazetat in 
1000 ec. Wasser unter Zusatz von 100 ce. Salpetersiiure (spez. Gew. 1.16), die 
als Elektrolyt bei der Bleiabscheidung diente. Als Elektroden dienten bei dem 
Versuch Stiicke aus reinem Blei. Diese -Bleistiicke bliehen nach der Elektrolyse 
etwa 3 Wochen in der Lésung stehen. Als ich sie alsdann herausnehmen wollte, 
bemerkte ich, dass sie ihre weiche, dehnbare Beschatfenheit véllig verloren hatten 
und eine spréde, bréckelnde Masse geworden waren. Der Gedanke, es hier mit 
einer stabilen Modifikation zu tun zu haben, erschien mir um so wahrscheinlicher, 
als das spréde Blei ganz dem grauen Zinn gleicht, beide Metalle zu der gleichen 
Gruppe des periodischen Systems gehéren und Metastabilitét unserer Metalle nach 
Ihren Forschungen nichts Befremdliches mehr ist. 

Kurze Zeit darauf brachte mir ein Kollege ein Bleikabel, das an verschiedenen 
Stellen eine weisse pulvrige Beschaffenheit zeigte von ganz ahnlicher Art, wie ich 
sie an den vorhergenannten Bleistiicken beschrieb. Wir machten darauf den Ver- 
such reine Bleistiicke unter konzentrierle Salpetersiiure zu bringen und sie mit ein 
wenig unseres spréden Bleies zu impfen. Der Erfolg blieb nicht aus: nach 
wenigen Tagen hatten sich betrachtliche Teile der Bleistiicke zu der bréckligen 
Modifikation verwandelt.” 

Mr. Hetiwr kindly invited us to continue these investigations ; 
repeating his experiments with our pure lead we were able to corro- 
borate his statements. 

12. The lead was melted, chilled in water and cut into small 
blocks (8,5 & 2 x 0,5 em.). We put them into glass dishes which 
were filled up with the solution mentioned by Henier. The dishes 
were covered with glass plates. The temperature of the solution was 
15°—20°. The addition of some nitrie acid has the effect that the 
surface of the metal remains bright during the experiment, 


In this way the electrolyte is in constant contact with the metal 
and the inoculation which occurs can go on undisturbed. 

The photographic reproductions (natural size) which accompany 
this paper illustrate the development of the phenomenon. Fig. 1 
shows a plate of pure lead in its original condition. Fig. 2 represents 
the plates after having been in contaet with the solution for some 
days; there are to be seen deep cracks, which show that the material 
has shrunk locally. In consequence of this an increase of the density 
was to be expected which was proved by means of the pyenometer 
(comp. § 19). Fig. 3 shows the plates after three weeks in the same 
conditions: the metal has been disintegrated. 

Repeating the experiment with 15 or 20 blocks we got in all 
cases the same results. 

13. We shall prove below that the phenomenon is not a chemical 
one; the following experiment may give already an indication in 
this direction. One of the blocks (+= 40 grams) was put into a cali- 


brated tube which had been filled up with the solution mentioned. 
This tube stood in a small dish containing the same solution. After 
three weeks no evolution of gas had occurred, either at room tem- 
perature or at higher temperatures. 

14. After this the phenomena described above were investigated 
by means of both the pyenometer and the dilatometer. 


A. Measurements with the Pycnometer. 


15. We exclusively used the instrument (Fig. 4) described by 
Apams and Jounston'), following the indications given by the authors. 
Moreover we took the precaution of dipping the pycnometer into 
water before weighing (empty) and wiping the 
water off with a dry cloth. If this is omitted a 
slight error occurs. as the surface of the pyenometer 
is then not in the same condition as at the sub- 
sequent weighings, after it has stood in a (water) 
thermostat. 

All determinations were carried out in duplicate 
with two pycnometers (C and D) which contained 
= 25 cem. 

16. Our investigations on bismuth, cadmium ete. 


had shown that the pyenometer measurements have 
to be carried out with special care. The volume 
changes which accompany the transformation of the 


1) Journ. Americ. Chem. Soc. 34, 563 (1912). 


826 


different modifications are, it is true, not inconsiderable, but they 
may be partially compensated in consequence of the simultaneous 
presence of different forms. In order to detect the remaining volume 
changes, very accurate determinations of the density must be made. 
We shall see below that special precautions must also be taken 
with lead. Evidently it is to be aseribed to such compensations that 
these phenomena have escaped the attention of earlier authors. 

17. We used toluene as a liquid in the pycnometer. 

Its density was found to be: 


9KO 


d —~ 0.86013 by means of the pyenometer C. 
4° . . 


0.86013 nimi 8 D. 


The quantity of lead used for each determination was 40—-60 
grams. The thermometers (divided into 0.05 degrees) had been checked 
against a standard of the Phys. Techn. Reichsanstalt at Charlotten- 
burg-Berlin. The weighings were carried out on a Bunex-balance 
with telescope. The weights had been checked by the method 
deseribed by TH. W. Ricuarps '). 

18. In the first place we determined (at 25°.0) the density ot 
the lead immediately after its preparation for the experiments. 
It was melted, chilled in water and filed to powder. It was then 
treated with a magnet in order to remove traces of iron from the 
file. We washed the powder with dilute nitric acid, water, alcohol 
and ether, and dried it in vacuo over sulphuric acid. Its density 
was now: 

gro 


av 
d 7 11.325, (Pycnometer C). 


The metal was then washed and dried again in the same way ; 
ORO 


d =e 11.322, (Pyenometer D). After treating again in this way we 


9FO 


a0 
found d ie 11.324, (Pycnometer D). 


19. We brought the metal into the solution of the acetate (temp. 
15°). After standing for 3 weeks the material was washed and 


95° 


dried. Its density was now d io 11.340, (Pycnometer C) 


11.3842, (Pvenometer JD). 


1) Zeitschr. f. physik, Chemie 33, 605 (1900), 


827 


The figures show that there has occurred at 15° an increase of 
17 units in the third decimal place. 

20. We put the metal again into the solution which was kept at 
50° (in a thermostat) for 120 hours. We found after washing and 
drying 


[> ral e} 


d = 11.313, (Pyenometer C 


11.312, (Pycnometer D). 


The density had decreased 28 units in the third decimal place. 
21. The experiment was repeated again, this time at 25°.0 (in a 
thermostat) for 144 hours. 


9ro 


We found: ie 11.327, (Pycnometer C) 


11.3829, (Pycnometer D). 


An tinerease of 15 units in the third decimal place had occurred. 
22. Our table I contains the results of these determinations: 


AT IN 18} VG EE 

252. 

d 40 

Without any previous treatment | 11.324 
After treatment at 15° 11.341 
s rf ee |} 11.3i3 

| 
” » n 25° | 11.328 


B. Measurements with the dilatometer. 


23. This investigation was carried out in the same way as has 
been described in the case of cadmium *). 

Some kilograms of lead were melted in a spoon and poured out 
into an iron form. The metal cooled in contact with the air. After 
filing it we treated it with a magnet and put it into the solution of 
the acetate. Here it remained (at 15°) for 15 X 24 hours. After this 
it was washed and dried in the way described above. We used 
+ 600 grams in the dilatometer. (Bore of the capillary tube 1 mm.). 


1) Proceedings 16, 485 (1913); Zeitschr. f. physik. Chemie 87, 409 (1914), 


828 


At 50°.8 the decrease of the level was 700 mm. (34 hours). 
5 74°.4 5p rise 9 % . ” 275 oo) ( DH ” Ns 


Whilst the first preparation (§ 20) had shown at 50° a decrease 
of density, we now find an imerease. From this result we may 
conclude that there are more than two allotropic forms simultane- 
ously present. 

24. Special attention may be paid to a phenomenon which we 
observed with all our preparations and which stands in close con- 
nexion with the fact that lead as it has been known up to the 
present, forms a metastable system containing simultaneously several 
allotropic modifications of this metal. 

It is generally known that when a bar of any metal which is 
more electro-negative (resp. electro-positive) than lead is suspended 
in a solution of a lead salt, the lead is thrown out of solution and 
a lead tree is formed. 

We found that the same phenomenon occurred when our pure 
lead was placed in the solution mentioned above or in a (neutral) 
solution of lead nitrate (30 grams of nitrate, 70 grams of water). 
Both at room temperature or at higher temperatures (50°) a lead 
tree was formed in a few days. 

25. We are in the case of lead in specially favourable cireum- 
stances for the observation of this phenomenon. The galvanic current 
which is generated between the stable and metastable modification 
decomposes the solution. The metal which is electrolytically deposited *), 
shows in this case a characteristic form (lead tree) so that the 
phenomenon is very striking *). 

26. We hope to report shortly on the different pure modifications 
of lead and their limits of stability. 


Utrecht, October 1914. van 't Horr- Laboratory. 

1) That the phenomenon is not to be attributed to the presence of iron (0.0006 
per cent) or copper (0.001 per cent) is proved by the investigations of OBERBECK 
{Wied Ann. 31, 337 (1887)] and by those of KénIGSBERGHR and MiLueER [Physik. 
Zeitschr. 6, 847 and 842 (1905). 

2) We also carried out an experiment with tin: white and grey tin were putin 
contact in a solution of SnCl, (Temp. 15°). After some time a great many 
beautiful crystals of white tin were deposited by electrolysis upon the white metal. 
(Comp. Ernst CoHen and E. Gonpscumipt, Zeilschr. fiir physik. Chemie 50, 225 
(1905)]. 


829 


Mathematics. — “On an integral formula of Stiuises.” By Prof. 
J. C. Kivuyver. 


(Communicated in the meeting October 31, 1914). 


In the Proceedings, and Communications, Physical Section, series 
3, 2, 1886, p. 210, Stivites treats of definite integrals, referring 
to the function 


Y= == 
‘ 1—y4 NI. 
In this function @ stands for a positive odd integer without qua- 


h 


a 


dratic factors, and ( ) represents LEGuNDRE’s symbol with the ex- 


tension given to it by Jacopt. 
nile 
As poles of the function f(y) only the points y=e* are to be 


taken into consideration, and for the residue, belonging to such a 
pole, one finds 


From the well-known fundamental equation 


ey ae 
> é a —7 2 sa Va 
h=1 a 

Qik 


it follows, that a pole is only to be found in those points y= e-¢ 
in whieh & is prime to a. Consequently y= 1 is not a pole of the 
function, and we have, 


1 '=a—1 /), 
hy) == Gz 
a h=1 a 


from which it follows that —«af(1) is equal to’the sum of the 
: h 
numbers smaller than «, for which @E- (residues), diminished 
a 
. . 4 : be 
With the sum of the numbers smaller than a, for which ( i — 1 
Ka, 


is (non-residues). 
In the paper quoted, Stipirsjus considers the definite integrals 
a 


<3) 
ee , tate: has. ata 
J (e—) sin da and aI f (e—*) cos dx, 
é 2a 7 2m 


0 0 


830 


and he calculates the value of the first integral for the case 
a= 4w + 1, the value of the second integral for the case 
a = 4w — 1. . 

In the following I give a shorter deduction for these results. 

I suppose that the two positive, otherwise arbitrary numbers 3 
and y have a for product, that ¢ is a positive parameter and now 
consider the integral 


pa file )aneas, 


In order to valeulate this integral, it is not necessary, as STIELTJES 
does, to fall back on an integral formula treated by Lecrnpre and 
by Aber. It need. only be observed that in the upper half of the 
complex v-plane for inereasing values of |.) the modulus of the 
integrand approaches sufficiently rapidly to zero, to permit us to 
equate the integral / to the sam of the residues in this upper half 
plane, multiplied by 222. 


Qnx 
The poles of the integrand are the poles of Fle 8 ie that is to 
E ki 
say the points z= —(#= 0,1, 2,:..), where & is prime to a. The 


” 


‘ 
residue of such a pole is 


1 h=a=1 AN * | 5 LN ea 
é / SS ) ¢ | ( = a 2 ) Va = || Uo 
2ay Swe any a 


hence 


a—| bey ees 7 _ 2akt a 1\2 a al 
eG, Pe i 2 ) > Ge v = 2 es 2 me a 
Y Nae Y 


We ought to distinguish now between the two cases a= 4w-+ 1 
and a = 4w — 1. 
For a= 4w-+1 we have 


is wey seals (a= 
ie) =-+ ( =) and consequently / C B ) =—f fe B ) ; 
a a 


so that it follows from the result found for J, that 


5 (ae /2 mee 
mc oe ree ee r). (c=40 - 1) ee) 
wv 2 
0 


On the other hand for a= 4w—-1 


h =) == = 
.) ——— (=) and consequently / (« i ) = +s(4 i ) : 
a a 


so that in this case it may be concluded from the integral formula that 


272 2rt 


a ; 2 
{ole ip ) cos 2zta da =} ye = if (« 7 ; oe (@ — 4A es (OL) 
wy Y 


0 


nh 
| 


As may be proved the equation (II) remains true if we suppose 
¢=0, and if the expansion in series 


2r2 2rmx 


: ee 10 “m ss 
PEALE B = 2 — | |e B ' 
M11 Nea 


is made use of, we get in this exceptional case 


m =e m\ 1 ae rd ha 1 fe) 
Ss -}|—= — f(1) = — > ( h. (a= 4w — 1) 
ee MO Ya aya j= a 


The results found by Stipitses have been derived with this, the 
equations (1) and (I]) may now, however, be used, to find other 
results less known in the theory of numbers. 

For real values of « the function / (e~**) has the property of approach- 
ing rapidly to zero for positive and negative values of x of increasing 
modulus. This leads. to the conclusion that Fourimr’s general sum- 
mation-formula 


is $x 
n=+an a n= 43 
=> F(§+n) =| F(y)dy +2 XS | F'(y) cos 2arn (y—&) dy 
1i—— © no 
as a 


may be applied, if we write 


(a) 7 aa 
£1 


Distinguishing again the eases a=4v+1 and a=4w—1, the 


Se 


and if we suppose 0< 


value of the integrals in the right-hand member may be determined 
by means of the equations (I) and (Il). It should be taken into 
consideration in the summations in the left-hand member, that / (¢-*) 
changes ifs sign together with « or not, according as @ is equal to 
dw +1 or to 4 — 1. 

In this way the two following general equations are derived from 
the summation formula. 


One sa 2n(n--5) 2rn(n—é) Y 
oF pt) n= ES ze SS Ee, 
ih (« B ) 5H i(- le ) ==) (- 8 ) = ] 
i) | : 
p n= Zan | 


he fae = sin sani (« 7 ) , (a= 4w + 1) 


7 n=!) 


Proceedings Royal Acad. Amsterdam. Vol. XVII. 


832 


p oa eee , _ onln-ts) ys 2n(n—F) \ 
! (’ i ) = i(< : ) : I (« : ) | = ] 
=| 


(IV ) 


7u=—= 


; ae Q7n 
as} t ray HED) SS cos Bank « 7 )| te 


Y n=l 

If in both members of these equations the functions / are expanded 
into series, the summations indicated are to be executed still further. 
1 shall, however, perform these reductions only for special values 
of the parameter §, in consequence of which the general results are 
simplitied. 

In the equation (IID) I substitute therefore §= 4, at the same 
time L replace 3 by g and accordingly y by 2y. I further write 


us T 
Be =f, Cin OKe 
The numbers g and g’ are then positive and smaller than 1; 
they satisfy the relation 
! m* 
log qex log ns 
a 
but are for the rest arbitrary. 


In this way the equation (III) passes into 


re 3B n= 
2S) (—1)" F (q+) — > (—1)" F(t), 
n=O of n—0 


and if the functions / are expanded into series, we shall find 


| ; 1 ne (“) qn rs | i ] ven (=) q” a 
oO” — ——<—<——— og a aid = = ToD a= w+l (V 
“ qG m=1 a) 14-92" i rj} 3d Qh ( ) ) 


In the equation (IV) I substitute $—=0O. We have then in the 
first place 


: no i /B é 1S As 
70) +2= Fq) =)" a) +25 70%, 
rm y N= 


and if again use is made of the expansion into series of the functions 
J we tind 


Vig | soya (2) 2. 
qd a y) = gFuc 


/, 1 Z LUE IL g2m / 
=! log ar) vay +23 ee ' (a = 4w—1) . (VI) 


qd m=1 \@ —q'2m 


The equations (V) and (VI) completely symmetrical with regard 
to y and gy’ are again conspicuous for the remarkable properties of 


833 


; m : Ae, 
the arithmetical symbol ( For the rest they show some similarity 
ct 
with f 


formulae in the theory of 


the functions, and point to a 


‘ ’ z 1 
certain connection between the functions & (« a) and or " 

{ Y 

So it may be observed, that, from the equation 

F 
ae A v, U, 
4 1 re it) B mn gq” 
Fe (ea See Se a 
p p 


—_= 4 = —— ¢os 22 mv 
a t m1 l--qm 
Dv, Osho 

p 


a la @ 
fe: ment rn ap 

Or 0, <7 vo, (Nee = = SS a 4 
B B h=1 r oe 


a 


e h 7 
1 i iN US ig . (| B 
VA vd, 0, | v, (0, | ve = 
i { 


— = \@ ae (a = 4w + 1) 
( 3) 
remains unchanged, if 3 is replaced by y 
In a similar way we conclude from 


(3) 
N v, — 
1 B 


m=o 
tA CA 


= (ple 

- otunm + 4a S ——— sin 2x mv 
U m=1 [—gen 

« 

(Pas = 
B 


for the case a= 4w —1 to 


7 ( | 
—=7— }) os a? We m= e6 27 
Le Banded Oot BOSH 

feat (a 1 PUVA) san Ye? a I= 

a ae 


m1 
We can prove now, that 


h=v—1 h ath 
>> ia 2Va Ff (1) 
h=1 a 
consequently it ensues from the aneaede (VJ), that the expression 
5 ic -) 
1 t=a—1 Sh ale a 
— 2 4 eS (a = 4w — 1) 
Vl jot NG € ,) 
a ee 
p 


holds its value, if 8 is changed into y 


on 
or 
* 


Physics. — “On unmiving in a binary system for which the three- 
phase pressure is greater than the sum of the vapour tensions 
of the two components.” By Dr. F. E. C. Scuerrrr. (Commu- 
nicated by Prof. J. D. van per WaAats). 


(Communicated in the meeting of Sept. 26, 1914). 


l.-In my investigation on the system hexane-water the remarkable 
phenomenon presented itself that the three-phase tension of the two 
liquid layers by the side of gas appeared to be greater than the 
sum of the vapour tensions of pure hexane and pure water‘). When 
the tensions of the pure substances at a definite temperature are 
denoted by P, and P,, the three-phase presstwe by /, then for 
temperatures which are not too far from the critical end-point 

| cae eee el a 

If we could speak of ‘partial pressures” for such an equilibrium, 
this result would be impossible. A proof of this is found in VAN DER 
Waats--Konnstamm’s “Thermodynamik’, which however is only 
valid when the gas-laws*) hold for the saturate vapours. When the 
vas-laws do not hold for the gas phases, in other words if the gases 
possess surface layers, the proof is not valid, and the statement that 
the three-phase pressure must always be smaller than the sum of 
the vapour tensions of the components, holds therefore only for 
rarefied saturate vapours. 

In my paper on the system hexane-water I have shown that the 
contradiction with the second law of thermodynamics, which at first 
sight may be supposed to exist in the observed phenomenon, is only 
an apparent one. We might, namely, be inclined to reason as 
follows: If the three-phase mixture possesses such a high pressnre, 
the pressure exerted by the water and hexane molecules, or at least 
that of one of them will have to be greater than the pressure of 
water vapour, resp. hexane vapour over the pure components. If we 
therefore bring the three-phase mixture by means of a semi-permeable 
membrane into contact with pure hexane and with pure water 
under their own vapour pressure, bexane or water will pass through 
the semi-permeable membranes from the three-phase mixture towards 
the pure liquid. We should then get splitting up of the three-phase 
mixture, whereas just on the contrary the so high three-phase pressure 
sets in of its own accord from pure water and pure hexane. This 
is in conflict with the second law of thermodynamics. 


1) These Proc. 16. 404. (1913). 
2) Thermodynamik. Il. S. 476. 


835 


I have shown in the cited paper that the conclusion that the 
three-phase mixture will expel water through a membrane permeable 
to water, is really correct, and that probably mutatis mutandis the 
opposite thing will apply to hexane. The error in the above reasoning 
lies therefore only in the very last conclusion. I have pointed out 
loc. cit. that it is, indeed, possible that two liquids, each under its 
own vapour pressure, mix to a three-phase mixture that possesses 
the property to get unmixed again into the pure components through 
semi-permeable membranes; that this is not in contradiction with 
the second law of thermodynamics, but that on the contrary this 
phenomenon will be frequently met with in my opinion, also for 
systems which do not present the special behaviour mentioned at the 
head of this paper. Thus solutions of gases which are but sparingly 
soluble in water will certainly expel water, when they are osmotic- 
ally brought in contact with pure water of the saturate tension. The 
observed phenomenon is therefore not in conflict with our theoretical 
considerations. 


2. To get an answer to the question whether the system hexane- 
water presents an exceptional behaviour in the appearance of a 
three-phase pressure which is greater than the sum of the vapour 
tensions of the components, I have investigated a number of other 
systems in the hope of findiug the remarkable phenomenon there too. 
First of all I have chosen the system pentane-water. The pentane 
which I had at my disposal, was however KaAHLBAUM’s ‘normal 
pentane’, which is no pure normal pentane, but a mixture of normal 
and isopentane, which can only be separated with great loss of 
substance and time, as the boiling-points of the. two substances lie 
near room-temperature, and differ only little (slightly more than 
8 degrees). This slight difference of boiling-point involves that the 
pentane mixture behaves pretty well as a pure simple substance; 
the isothermal pressure ranges for condensation are slight. I have 
therefore given up the separation of the two pentanes, and compared 
the vapour tensions of the pentane mixture and of pure water with 
the three-phase tension of a pentane-water mixture. It is clear that 
both the pentane mixture and the three-phase mixture must possess 
a tension dependent on the volume at constant temperature, but 
also the three-phase tension appeared to be only little dependent on 
the volume. To execute this comparison of the pressures as exactly 
as possible I have determined the pressures for final condensation 
and for about equal volumes of gas and liquids both of the pentane 
mixture and of the three-phase mixture. 


836 


TABLE I. 
a i = al | 
| 
Pentane mixture. 
| Pressure (atm.) 
Tem | =i a | 
| -, | 
perature. Erle : | 
V, =V 
condensation L G | 
51S) es M65 | 
| 
| 151.9 | 17.8 | 
161.1 20.6 | 
| 
161.45 20.8 | 
169.95 Pele | 
170.1 | 23.7 
180.1 21.6 | 
180.3 27.8 \\ =a) 
| 190.25 32.15 | 
| | | 
i 400.30" i sS205).5 ul 
| 193.3 | 9) 33:6 


TABLE II. 
Threephase mixture. 
Pressure (atm.) 
Tem- 2 a 
perature. Ende 
Vi Va 
condensation| 4 G 
150.15 22.45 
150.7 22.7 
160.6 27.25 
160.7 27.35 
166.5 30.3 
170.25 32),55 
170.35 32.65 
180.3 39.0 
180.5 3925 
| 
187.1 44.1 


When the values of pressure and temperature indicated in the 
above tables are graphically represented, it appears that the line 
for the end-condensation coincides fairly well with that which holds 


for 


equal liquid and vapour volume both for the pentane mixture 


and for the three-phase mixture: the difference is nearly everywhere 
smaller than O.1° atmosphere, and 


is therefore of about the same 
value as the errors of observations. When the pressure values are 
read for definite temperatures from the graphical representation, the 
values of table 3 are found. 


IWAVBsL ET 
| oe Three-phase | Pentane | ; 
Temperature | pressure pressure Waterpressure | Difference 
— _— — —_—____—_- —_ ————_——— | ————— — — == 
150 22.4 7s} 4.7 0.4 
160 27.0 20.3 6.05 0.65 
170 32.4 23.7 7.8 0.9 
180 38.8 27.6 9.8 1.4 
187.1 44.1 30.7 11.6 1.8 


The values for the vapour tension of water lave not been derived 
from earlier observations, but determined by myself to prevent an 
eventual deviation of the thermometer from vitiating the comparison. 
All the observations have been carried out with a normal thermo- 
meter, and with an Anschiitzthermometer verified by the boiling 
point of pure aniline. 

We draw the conclusion from the last column of table 3 that 
the three-phase tension is again greater than the sum of the vapour 
tensions of the pentane mixture and of pure water. The difference 


appears again to. be greatest at the critical endpoint —— in all thie 
tables the critical values are printed in bold type —; with decrease 


of temperature the difference decreases rapidly, and according to 
the theory it must reverse its sign at temperatures where the saturate 
vapours follow the gas laws. 

The above described example shows therefore again a case of 
very high three-phase pressure. Though these experiments would 
have to be repeated with the pure substances to get perfect certainty 
about the behaviour of the binary systems, the conclusion that the 
pentanes and hexane behave analogously with respect to water, 
seems yet sufficiently certain to me. Also the relative situation of 
the critical end point with respect to the critical points of the com- 
ponents is the same as for the hexane-water mixtures. 

Finally I will still point out that the above only proves that there 
exists a pentane-water mixture that possesses the repeatedly men- 
tioned remarkable property, and this suffices also for my purpose ; 
other proportions of pentane mixture and water will probably give 
rise to some change in the three-phase tensions because the pentane 
mixture is not a simple substance; for the solubilities of the two 
pentanes in water will probably not be in the same proportion as 
the quantities of the pentanes in the pentane mixture; the difference 
in the fifth column can therefore undergo some modification for 
another ratio of the two “components”. 


§ 3. The experiments of § 2 confirming my supposition that the 
abnormal value of the three-phase pressure would be a phenomenon 
of frequent occurrence, | thought I had a great chance to find the 
same peculiarity also for other binary systems. I have therefore 
looked for binary systems of which it was known that for low 
temperatures the threephase pressure lies higher than the vapour 
tensions of the pure components separately and is about equal to 
the sum. Dr. Bicuner drew my attention to the systems carbon 
tetrachloride-water and benzene-water, which possess three-phase 


838 


tensions according to Rrexavir, which deviate little from the sum 
of the vapour tensions of the pure substances. ReGNauLT even asserted 
that the tension of carbon tetrachloride-water mixtures is somewhat 
higher than the sum, and thought he had to ascribe this to slight 
contaminations; GerNpz has shown later that the three-phase tension 
is really slightly smaller than the sum of the vapour tensions, which 
is therefore in harmony with the theory. I have now tried to inves- 
tigate the two systems at higher pressure; I have, however, not 
succeeded in doing so with the system carbontetrachloride-water, as 
the components act on each other at higher temperatures. The inves- 
tigation is possible for the system benzene-water, and also this system 
appeared really to furnish an example of the remarkable phenomenon. 

Benzene free from thiophene (negative isatine reaction) was distilled 
from phosphorus pentoxide; the boiling point under normal pressure 
was 80°.2, and was therefore in perfect concordance with the value 
given by Youne. The vapour tension line of this benzene was deter- 
mined, and then the three-phase tensions of a benzene-water mixture 
were measured and compared with the vapour pressure line of water, 
which was also determined by the aid of the same thermometers. 
To avoid corrections I have measured the three pressure values 


TAB ie AV: 
Temperature | Bo | Waterpressure | re | Difference 
0 
150.0 10.6 | 4.7 5.9 0 
160.0 13.2 | 6.05 Tht 0.05 
170.0 16.4 | 71.8 8.5 0. 
180.0 20.1 | 9.8 10.2 0.1 
190.0 24.6 12.35 12.15 0.1 
200.0 29.8 15.3 [OS aks 0.2 
210.0 | 35.9 | 18.75 | 16.7 0.45 
220.0 | 42.9 | 22.8 19.45 0.65 
230.0 50.9 | 27.5 22.5 0.9 
2AO ele Ne e602355 9/0 8330 25.95 1.4 
250.2 | 70.65 | 39.1 | 29.55 | 2.0 
260.1 82.15 | 46.1 | 33.7 | 2:35 
967.82 dul ok ode7 ‘cale.(52.4) ‘cale.(37.35) 2.95 
268.2 | = 52.6 37.5 — 
| = 


839 


always at the same temperatures; if a slight error should occur in 
the absolute value of the given temperatures, this has no influence 
on the pressure differences. The thermometers which I used in this 
investigation, have been tested by a resistance thermometer, the 
resistance of which was determined for boiling water, naphthaline, 
benzophenon, and sulphur. The obtained results are given in table 4, 
the pressures are given in atmospheres. 

It appears from the last column of table 4 that the difference at 
150° to 200° is only slightly greater than the errors of observation, 
that the three-phase tension becomes appreciably greater than the 
sum of the vapour tensions at 210°, and that this difference rapidly 
increases with ascending temperature. 


4. When we combine the results of the system hexane-water 
and those of § 2 and 3, it appears that in the three systems the 
three-phase tension is always greater than the sum of the vapour 
tensions of the components in the neighbourhood of the critical 
endpoint. Moreover these three systems present the same shape of 
the plaitpointline in the 7-x-projection; the upper critical endpoint 
always lies lower than the critical points of the two components ; 
the plaitpoint line presents therefore a minimum temperature in the 
T-x-projection (homogeneous double plaitpoint). Though in my opinion 
it is probable that the systems will behave perfectly analogously, a 
furtber investigation would have to decide whether for all this 
homogeneous double plaitpoint lies in the metastable region; | have 
shown this for the system hexane-water in my cited paper. It is 
remarkable that in the system ether-water the homogeneous double 
plaitpoint appears in the immediate neighbourhood of the ether axis 
or would perhaps lie outside the figure, so that the eritical endpoint 
in contrast with the above discussed systems lies between the critical 
points of the components. In this system the said peculiarity does 
vot occur. Accordingly I think I have to conclude that the systems 
which present critical endpoints which lie lower than the critical 
temperatures of the two components possess three-phase pressures 
which are higher at high temperatures than the sum of the vapour 
tensions of the pure substances, whereas the opposite is the case for 
systems for which the critical endpoint lies between the critical 
temperatures of the components. Perhaps this conclusion may contribute 
to account for this remarkable phenomenon. 

Anorg. Chem. Laboratory of the 


June 25, 1914. Ae : : 
University of Amsterdam. 


840 


Physics. — “Contribution to the theory of corresponding states.” 
By Mrs. T. Exrunrest-Aranassyewa. D. Se. (Communicated by 
Prof. H. A. Lorentz). 


(Communicated in the meeting of September 26, 1914), 


§ 1. Mestin') has tried to demonstrate that every equation of 
state which contains the same number of material constants as 
variables, is to be reduced to a universal shape (.e. to sucha form 
that no parameters occur any more which vary with the substance), 
if the variables are replaced by their relations to suitable special 
values, which may be designated as “corresponding” for different 
substances. 

On closer investigation it appears, however, that the equality of 
the number of the parameters and that of the variables is neither 
necessary nor sufficient for the existence of corresponding states. 

A method will be given here to decide whether a given equation 
allows the existence of corresponding states. This method furnishes 
at the same time the possibility to calculate the eventually corre- 
sponding values of the variables for different substances. 

§ 2. In the first place we shall define the term ‘corresponding 
states” in a somewhat more general form. Let an equation be given 


between a system of nm variables: 7,,.v,,...%, and a number m of 
such parameters: C\, C,,...C, that they can vary with change of 


definite circumstances (for evample of the substance). 

Let an arbitrary system of special values: 2,',2,',...2,' (we shall 
briefly denote it by a) of the variables 2; be known, which satisfies 
this equation for definite special values C;' of the parameters C;. 

Let us introduce the following new variables: 

a, vs &y 


R= RS Se = = 
2, vy an 


ee (ik 


All the constants S; of the thus transformed equation ean be 
calenlated as functions of the former constant coefficients, of the 
values Cy) and of the values 2,/. 

When the parameters C; assume other special values C;", other 
systems of special values of the variables will satisfy the original 
equation. 

The case may occur that there is among them such a system of 
values : 


}) Mestin: Sur lVéquation de vAN DER WAALS et la démonstration du théoréme 
des élats correspondants C.R. 1898, p. 180. 


S41 


" 


. PL roy ht 
Uy Uy 02+ Uy 


that on the substitution of 


for vi, the constants of the transformed equation assume exactly the 
same numerical values S; as in the first case. We call such values 

Na ae Vat ald: thie 
state defined by the values 2;", correspondent to that defined by the 


! 


a .t, correspondent to the values x,', x, 
1? 


M1 9 Ug yee 


values a; (or corresponding to it). 
The form to which the given equation is reduced in this case 
XL vi 


by the substitution y; = —, resp. yi= — 


will be indicated by the 
Xi vi 


word universal. 


§ 3. When for the system a; the system 2; corresponding to it 
has been given, the system aj" can be easily caleulated, which cor- 
responds with every other system 2’ of ; values, which satisfies 
the equation in the first case, by the aid of the following equations: 


Indeed the values 2;' resp. v;" satisfy the original equation, when 
the parameters C; assume in it the values (;' resp. Ci". When now 
the substitution 


ABS P 
ee ee ke ee 28) 


=f 

vi 
has been earried out, the constants S; which we have calculated, 
assume other values, e.g. S41, and we must now find the values 2", 


oD 


it) 


which keep the quantities Sj, invariant on substitution of Gy tom Ge 
when the substitution : 


hy 


i Geet ies) oo Gaetan ca) 
LY 
is carried out. 
The values x;', however, satisfying the given equation, 
; Qe 
ya =, 
ly 
satisfy the transformed equation. The constants of the transformed 
equation do not change, when 


ll 9 f 
av; Vi 


" ! 
Ly Li) 
is substituted for Yar: 


842 


The fraction: 


" t 
2; wey 


wi" wit! 
belongs therefore to the corresponding values ;", hence wv’ corre- 
sponds to ay". 

Hence it is proved that im the case of a system of values corre- 
sponding to a system of solutions, there also enists a system corre- 
sponding to every other system of solutions (when C;’ have been 
replaced by C;"). 


§ 4. To find a system «;", if the system x,’ has been given, we 
take into account every product of powers of the variables: 
[OR (OES og 0 F Bain. <0 
which appears as separate argument in the given equation. We 
shall therefore write the given equation as follows: 
@(K,P,, K,P,,..:: KePpj Ly Dy. 0. ti) = 0 
K; and LZ; are constants with relation to 2;, Z; are those constants 
which do not oceur as factor of Pi, but in any other way. Among 
the A; and Z£; are therefore also included the variable parameters 
(for their funetions). 
Let us put that the constants A;, 4; in the first, resp. second case 
have the special values: 
K;', 0’, resp. Ky", 1," 
(those among them which are independent of C;, have the same 
values in both cases); they are to be considered as given. We can 
write every variable also in the following way : 
CS ge —— ie Yi- 
(05 
If we put them in this form in the equation (7), it assumes the 
following form: 
D(Qi Pina. 2 Qe Lay) oe) 0 (8) 
in which 


Q) Kp! vo: ee 
Pg JOA gp (002 aon Pee (10) 
P:(y) = y ol yt? Wane yn tin Se (11) 


Now it is evidently the question to find such values z;" that when 
Ci' is replaced by Ci" and «2;' by @;", all the constants Q; and ZL; 
— eventually with the exception of one factor, by which all the 
terms of the equation can be divided — assume the same values. 


843 


When we carry out this division — let the factor in question be 
FR (it can be both one of the Q, and one of the Z;) in all A+/—1 
constants remain, which can have four different forms: 


ee : lca 
The required 2;" must now satisfy the following equations: 
Q = &" 
Siena 
RR eae ee) 
L;' L;" 
Ses ae 
and besides the following equations must hold: 
Eko a eee titantron att). TLS) 


The number of equations (12), in which 2;" occurs, is quite 
independent of the number of mm of the variable parameters C;. 

When all equations (13) are satisfied, and all those among the 
equations (12) which do not contain a;", the three following cases 
can occur. 

1. Equations (12) are in conflict with each other (a group of s 
of the sought values is defined by more than s independent equations. 

2. They have one, or a finite number of systems of solutions. (It 
is required, though not sufficient for this that the number of independent 
equations in which 2;" occurs, is equal to xn. Hence m must not be 
greater than 7). 

Which of the systems of solutions corresponds with the given 
system ;', has to be decided by a further investigation in every 
separate case. 

This is the case in which we have corresponding states. / 

3. They have an infinite number of systems of solutions. (It is 
required for this that m is greater than the number of the equations 
that are mutually independent). In this case we may speak of corre- 
sponding states for the same conditions (e.g. for the same substance). 


§ 5. We shall now examine how Mesuin has come to another 
conclusion. Mersin starts from the conviction that all the constants 
of an equation are independent of the choice of the unities, when 
every variable in the equation bas been divided by a special value 
of it. This is perfectly correct. It is also true, as we have seen, that 
every equation can be reduced to a form as meant here. 

It is however not true that those constants that do not change 
throuyh exchange of the unities, would also have to be unive. sal. 


S44 


Mrstin seems to be not quite free from a confusion, which is indeed 
pretty widely spread: between the change of a number occurring 
in an equation through change of unities, (“formal” change) and its 
change through transition to other conditions (to other specimens of 
the quantities which are measured by this number) (‘“‘material” 
change). 

In connection with this the assertion that in case of an equal 
number of variables and parameters the latter can always be com- 
pletely expressed in the former, is to be rejected. 

§ 6. We shall illustrate what we have discussed by examples, 
which though fictitious, are as simple as possible. Their claim to 
physical signification, can indeed always be vindicated in this way 
that they are interpreted as equations for the geometric shape of 
some physical system. 

1. y=ar’+ea+t+d QS23,. i=): 

a. Introduction of special values of the variables 


y BNE a 
Yo == ax,” rs ap vo =F b 
0 


Yo ey ‘ 


6. Division by @,=¥,: 


y Dal ac a ae b 
Foes (joe =) |) fe SS Sh 
Yo Yo vy Yo Xo Yo 


c. Determination of the numerical values of the special values 
of the variables satisfying the equation and of the coefficients : 


1 
i ; ie—=10 
a 
ax,” 1 
Yo ab 
L, 1 
Yo ab 
b 
3S) Ile 
J) 
d. Determination of the system of corresponding values : 
ign l 
— — 2 ! 
Yo. ab Y= 
ae. 1 , b! 
= — — i 
yo! ab H ab 
b i Hep. capley 1 
ale Me ath? ab’ 


845 
from which would follow that a'b'! = ab, whieh would be possible. 
only when we have really but one independent parameter. 
It follows, however, from the thesis of § 3 that if for one system 
of solutions there is not to be found a corresponding one, there 


does not exist one for any other system of solutions. 
Hence the given equation cannot be reduced to a universal form. 


2. y=au? + abe + Db? (oh 2n rt 2) 
D BENE a i 
a Yo — =@e, + abe, — + b? 
Yo a oe 
b yo wef“ aby,c 6 
ae aio ve 
Yo Y 0 a 0 Yo a 0 Yo 
‘ —b 
t ys? : “= — 
a 
Gnas ae b? 
—— = | c i) = i : = = | 
Yo Yo Yo 
' ! b 
d ye — 02 Co 
a 
3. y Save? +e (rol) 
D az \* a 
a Uy = = Ge || I) Sa ae 
Yo x4 & 
5, y vei ain (Z i ae eh 
Yo Yo vo Yoo 
1 2 
C. e, = H y= 
a a 
dine 1 ip. I 
=- ; —-=- 
Y «4 Yo 2 
1 9 
d i ; y= 
; — : a 
a a 
41). pu=A+t BIT CT? (35, 12 3) 
Pp v En ah bs 5 pp 2 
a. Po% —— =A -f Blo TCL, r 
Poo 0 0 


Gmp Diplo! ct A Al: BSB as Cie = OT. 


B : C 
As 7 independent of Cc T,*, the two last comparisons are contra- 


dictory, so that even if A= A’, we should not have corresponding 
states. 
Leiden, August 1914. 


1) This example fails in the Dutch text. 


846 


Chemistry. -— “The nitration of the mixed dihalogen benzenes”’. 
By Prof. A. F. Honieman. 


(Communicated in the meeting of Oct. 31, 1914). 


When in benzene are present two substituents and a_ third 
is introduced, the substitution velocity caused by the two groups 
already present is unequal. From the data given in the literature 
it may be deduced that those velocities for the substituents poimting 
to the p-o-positions decrease in the subjoined order: 

OH > NH, > halogens > CH,. 


The question now arose how to express those velocities also in figures. 

Dr. Wipavut has done this for chlorine and methyl by determining - 
in what proportion the isomerides are formed in the nitration of 
o-chlorotoluene. In this compound the positions 4 and 6 are occupied, 
under the influence of methyl, by a nitro-group, the positions 3 and 

OU, 5 under the influence of chlorine. If now we determine 
Ns the proportion in which the mononitro-chlorotoluenes 4 —-+ 6 
L ; are present in regard to the isomerides 3+ 5 in the 
N nitration product, this is then also the proportion of the 
substitution velocities caused by methyl and chlorine, because they 
can exert their action in this o-chlorotoluene independently of each 
other; for the positions which are substituted under the influence 
of methyl are different from those that ave substituted under the 
influence of chlorine. For this proportion was found CH, : Cl=1: 1.475. 

Dr. vAN pen AruND had previously determined the proportion in 
which the nitro-p-chlorotoluenes are formed in the nitration of p-chloro- 
toluene. If now, with the above mentioned ratio, we calculate the 
relative quantities, those calculated figures appear to agree approxi- 
mately with the observed ones. 

These researches, carried out in my laboratory, have now been 
continued, partly by Dr. Hrinkken, so as to determine also the ratios 
of the halogens. The method followed previously for the quantitative 
determination of the isomerides, namely by means of the solidification 
curves, could, however, not be applied here as the two nitro-p- 
chlorobromobenzenes give a continuous series of mixed crystals and 
because it was to be expected, on account of the fact that the 
properties of the nitrodihalogen benzenes present a strong mutual 
resemblance, that this would oceur in other cases also. 

Hence, for the quantitative determination of the isomerides present 
in the nitration mixtures, we made use of the property that a halogen 
in nitrohalogen benzenes is taken from the nucleus by Na-methoxide 


S47 


only then when it is placed in the ortho- or the paraposition in 
regard to a yee Of the isomerides 


aes Ds Br ie iy 


Ome ne | Iv 
oe 


3r NOs 


val 


I, IV and VI only chlorine, of If, IIL and V only bromine will be 
replaced by OCH,. Hence, if we determine the proportion in which 
chlorine and bromine are split off from the nitration product of 
p-chlovobromobenzene and trom that of o-chlorobromobenzene, we 
get at once the proportion wherein in the first nitration product 
I and II are present in the second one IV + VI on one side, UI + V 
on the other side. This method has also the considerable advantage 
that all the isomerides for the construction of the fusion lines 
now need not be prepared individually and that in the nitration 
products the various isomerides need not be separated; this latter 
attempt in particular would, presumably, have failed owing to 
insuperable obstacles. 
The results obtained are as follows 


Nitrationproduct of p-chlorobromobenzene contains 45,.2°/, of the 
Cl 


JNNOz 


compound | ; and 54.8°/, of the isomeride 1, 3, 4. 


NZ 
Br 


Cl cl 
Br NO, Bi 
Nutr. product of o-chlorobenzené consists of 55.5°/, of + 
NO, 


T\ ne 


th | ; orin molecular proportion 1 :0.80, 


Ye NON 


The substitution velocity caused by chlorine and bromine when 


and of 44.5°/, of 


present together in the benzene nucleus is therefore as 1: 0.80. 
When caleulating this proportion from the composition of the nitration 
product of p-chlorobromobenzene it must be remembered that in the 
nitration of chlorobenzene there is formed 30.1° , of the o-compound, 
but in that of the bromobenzene 38.3°/, of the same. If we eall 
wv the ratio of the velocities caused by chlorine and bromine we have 
30.1 : 38.382 = 45.2 : 54.8, 
ob 
Proceediugs Royal Acad. Amsterdam. Vol. XVIL 


S45 


from which «= 0.96. Hence, the result is here Cl: Br = 1: 0.96, 
The mean result of these two experimental series is therefore: 
Cle Br sAOrSse: 

The nitration of p-chloroiodobenzene caused the separation of large 
quantities of iodine with formation of p-chloronitrobenzene. Hence, 
for my purpose it was unsuitable. 

In the nitration of o-ch/oroiodobenzene, there was also some separation 
of iodine, but the formation of o-chlovonitrobenzene did not amount 
fo more than about 3°/,. When determining the proportion in which 
Cl and I were separated from the nitration product by NaOCH, a 
correction for this must therefore, be applied. For the velocity ratio 
Cl: 1 was thus found the mean value of 1:41.84. 

It now became interesting to also investigate the nitration product 
of o-bromoiodo benzene quantitatively as to its components. For, as 


Cl: Br was found —1:0:80 and Cl:1=1:1.84, Br:] should 
be = 1: 2.80, if indeed the two halogens present, aet quite indepen- 


dently of each other. 

Also in this nitration a little separation of iodine took place; the 
content of o-bromonitrobenzene in the nitration product was in 
this case 4.4°/,. Applying a correction for this the mean ratio 
Br: 1} 1:1.75 was found, which rather differs from the calculated 
figure. If, however, we caleulate the percentages of the isomerides 
with the ratios 1.75 and 2.380 the theoretical value gives 69.7°/, of 
the isomerides Br, 1, NO, = 1, 2,3 +1, 2,5, and the experimental 


value 63.6°/, which may be considered as a sufficient approximation 


0 
if we bear in mind the difficulties of these quantitative determinations. 

The conclusions from the above are obvious. Since it has 
appeared that two substituents simultaneously present in ortho- and 
in parapositions do not sensibly interfere with their respective 
actions in regard to a third entering group, we shall be able to 
calculate from the figures now found with sufficient probability in 
What proportion are formed the isomerides of other compounds, for 
instance in the nitration of o- and of p-bromotoluene. 

The above mentioned order of the substituents towards the decreasing 
substitution velocity caused by the same now becomes : 


OH > NH, >I >Cl> Br > CH,. 


Hence, the ratio OH: NH, and NH,:1 still remains to be deters 
mined. As, however, in the nitration of the iodoanilines great diffi- 
culties may be expected, A. F. H. Losry pr Bruyn has taken 
in hand a quantitative research of the nitration of o- and p-chloro- 
aniline in the above direction. As a preliminary result of his experi- 


849 


ments it may be mentioned that the ratio Cl: NH, is very large. 
The above velocity series must, therefore, be resolved into two parts: 
OH and NH, which cause a great substitution velocity and which 
are presumably of the same order of magnitude; on the other side 
the halogens and CH, with a lesser velocity, also of the sanie order 
of magnitude. A more detailed deseription of the above experiments 
will be published in the Recueil. 


Oct. 714. Org. Chem. Lab. University Amsterdam. 


Physics. — “The reduction of aromatic ketones. U1. Contribution 
to the knowledye of the photochemical phenomena.” By Prof. J. 
BorseKen and Mv. W. D. Congnx. (Communicated by Prof. A. 
F. Honinman). 


(Communicated in the meeting of October 31, 1914). 
I. The reduction of the aromatic ketones in a perfectly neutral medium. 


In our former communications?) we have shown that the reduction 
of the aromatic ketones does not proceed any further than to pinacone, 
which is presumably formed from the primary generated half pina- 
cone molecule by vapid polymerisation. The fact that in an alkaline 
medium hydrol is always obtained, must be attributed to the rapid 
transformation of the pinacone, under the influence of the hydroxyl- 
ions, into an equimolecular mixture of hydrol and ketone, the latter 
of which can be again reduced to pinacone. 

This explanation was confirmed by the study of the reduction of 
ketones by means of aluminium amalgam. 

Here is formed a mixture of pinacone and hydrol; the proportion 
in which these two substances are formed differs from ketone to 
ketone and now it appeared that the quantities of hydrol ran strietly 
parallel to the velocities with which the diverse pinacones are con- 
verted into a mixture of ketone and hydro! under the influence ef 
sodium ethoxide. 

Hence, aluminium amalgam in 80°/, alcohol may by no means 
be considered as a neutral reducing agent. 

The only modus operandi that gives the necessary guarantee that 
complete neutrality would prevail during and after the reduction is 
the action of the aromatic ketone on an alcohol under the cooperation 
of sunlight. The original intention of this part of the research, 


1) Proc. XVI. p. 91 and 962 (1913). 
56* 


$50 


namely the tracing of the progressive change of the reduction, was 
soon attained by applying this method. 

A series of ketones dissolved in a great variety of alcohols and 
a few other substances, was exposed to sunlight (or to the light of 
the quartz-lamp); dn all cases where reduction set in, not a trace of 
hydrol was obtamed. 

The ketone was usually quantitatively converted into pinacone ; 
occasionally, namely with benzylaleohol and a prolonged exposure 
to sunlight a combination of the half pinacone molecule with a 
eroup of the benzylaleohol, namely triphenylglycol was obtained as 
a by-produet. *). 

When to the aleohol some ethoxide was added hydrol was formed, 
as was to be fully expected. 


Hence, we arrive at the result that in the reduction of aromatic ketones 
the hydrogen unites exclusively with the oxygen. 


The experiments were carried ont as follows : 
Quantities of 5 grams of the ketone were dissolved in 50 ce of 


2 


alcohol rendered carefully anhydrous *) and exposed in sealed tubes 
of common glass to direct sunlight. 

The drying of the lower terms was performed by successively 
boiling with CaO, allowing to remain over metalli¢ calcium at O°, 
and distilling; the higher ones were purified by distillation and both 
were then immediately sealed into the tube together with the ketone. 
After exposure to the light for some time, during which the course 
of the reduction could be traced by noticing the deposition of the 
sparingly soluble pinacone, the tube was opened, the pinacone was 
filtered off, the filtrate distilled, the residue united with the pinacone 
and in the distillate the aldehyde or ketone was tested and in 
some cases determined quantitatively. 

The exact details will be published elsewhere by one of us, a 
few remarks may suffice here. 

First of all was investigated the behaviour of benzophenone in 
regard to methyl, ethyl, -propyl, sec.-propyl, cso-butyl, n-heptyl, 
sec.-oetyl and cetylalcohol. The latter only was not attacked, not 
1) This had already been noticed by Cramrctan and Sitper (B. 36, 1577 (1903)) ; 
the formation thereof is moreover a confirmation of our conception that as the 
first reaction product the half pinacone molecule is formed. 

*) Water acts in this reaction in a remarkable manner as a powerful negative 
catalyst; in 80°, alcohol no reduction takes place after exposure for months, 
whereas in absolute alcohol in the same conditions, about two grams of pinacone 
are formed during ten hours’ action of sun-light. 


851 


even at higher temperatures ; the mixture however, was of a fairly 
strong yellow colour. 

The other alcohols reduced the benzophenone in some sunny 
spring days, with the exception of methylalcohol which required a 
much longer time. 

The research was then continued with allylalcohol, geraniol, cyclo- 
hexanol, benzylealeohol, phenylmethylaleohol, benzhydrol and cinna- 
mylaleohol. Of these, the saturated alcohols reduced rapidly and 
quantitatively ; the allylaleohol was attacked more slowly with form- 
ation of acraldehyde (even after two months’ exposure to light, the 
acraldehyde was unchanged, thus showing that the light alone does 
not exert a polymerising influence on this mobile substance). 

The geraniol was also oxidized very slowly, the cinnamylalcohol 
remained unaffected (we will refer to this behaviour later). 

A few tertiary alcohols were also investigated; if was expected 
that these would remain unaffected and indeed this was the case 
with the dimethyiethylearbinol after two months’ exposure; during 
that period, diaethylmethylearbinol had generated 0,38 gram of pina- 
cone; with methyl-di-nu-propylearbinol the separation of pinacone 
started after a few days and after two months 0.7 gram bad formed. 

From this we notice that when the chain becomes longer, the 
activity of the hydrogen of tertiary alcohols gets enhanced, which 
enables it, with the cooperation of sun-light, to attack an aromatic 
ketone; what gets formed from the alcohol has not been investigated 
by us. 

From observations of Ciawician and SiLBer') it is known that the 
hydrogen of some hydrocarbons, such as toluene, is already active 
enough to cause this reduction. We have been able to show that 
also the hydrogen of the cyclohevane is transferred to the ketone, 
on the other hand, hydrogen itself was not capable of acting. 

Besides benzophenone some other ketones — particularly those 
that. were previously subjected by us to the action of aluminium 
amalgam — were subsequently exposed in alcoholic solution to 
the light. 

Nothing but pinacone was ever obtained, but the phenomena 
occurring in these photo-reactions induced us to systematically repeat 
a large part of these purely qualitative observations in such a manner 
that on using a very simple modus operandi a relatively-quantitative 
result was still obtained. 


1) B. 48, 1537 (1910), 


Il. The photo-reaction: ketone +- hydrogen'= pinacone. 

In order to obtain a relatively-quantitative result we could make 
use of a constant source of light and allow this to act on the differ- 
ent solutions under the same conditions; for this purpose a small 
7 em. quartz-mercury lamp was at our disposal. Yet we have em- 
ployed this method but rarely, for instance in continuous dark 
weather, because on account of the unequal distribution of the light, 
at most two little tubes could be placed in front of the lamp in 
such a manner that it might be assumed that they existed under 
equal conditions. 

When it had been ascertained by us that the reduction took place 
quite as well in ordinary white glass as in quartz, from which it 
appeared that a very large part of the actinie rays was situated in 
the visible spectrum, the experiments intended for comparison were 
carried out as follows: 

A number of equally wide tubes of the same kind of glass and 
having walls of approximately the same thickness were filled with 
the same quantity of solution, and all placed at the same distance 
in front of a white screen, which was placed close to a large labora- 
tory window. 

In this manner it was attained that the quantity of light that 
fell in the same time on each solution was practically the same, 
and perfectly comparable results were thus obtained. s 

It speaks for itself that even then only the figures of a same 
experimental series were mutually comparable. *). 

A photo-reaction is distinguished from a reaction in the dark by 
two points. 

It is of a lower and frequently of the O order in regard to the 
substance which is being activated and the temperature coefficient 
is smail. *) 

As we found that the active light was situated in the visible 
spectrum and that the alcohols do not absorb visible rays, the 
ketones are in this reaction the sensitive substances, and so we could 
expect that the quantities of pinacone would be independent of the 


1!) Also comp. O. Gross Z. phys. Gh. 37, 168 (1901) and E. GoupBere Z. phys. 
Ch. 41, 1 (1902). 

*) The first property is due to the activation occurring in the outer layer; from 
the sensitive substance only a limited number of molecules can be raised by the 
same quantity of light to the same degree of activily; even at a moderate dilution, 
the reaction becomes, on this account, indevendent of the concentraticn of the 
sensitive substance and therefore of the O order. This applies to slowly progress- 
ing veactions where the sensitive substance can be rapidly supplied by diffusion 
frora the dark interior to the light zone. 


ketone concentration (in regard to the sensitive substance a reaction 
of the O order). 

By selecting the alcohol itself as a solvent the change in con- 
centration thereof could be eliminated. (Table 1). 

In order to determine the order of the reaction in regard to the 
alcohol, benzene was chosen as being a general, non-absorbing and 
non-reducing solvent. (Table Ia) (Chronologically these last experiments 
were made after the position of the active light in the spectrum 
had been ascertained; we, however, state them here because they 
enabled us to give a complete image of the course of the reaction.) 

We notice that this reaction is indeed independent of the con- 
centration of the ketone, but not independent, however, of the con- 
centration of the aleohol. As the quantities thereof had been chosen in 
such a manner that they were amply sufficient even at the slightest 
concentration, it follows from the figures obtained that the velocity 
of the pinacone formation is proportional to the concentration of 
the alcohol. *) 

Thus we may represent the reaction by the kinetic equation : 

Mpinacone) = K L, [Alcoh.| 
dt 

With a constant light-quantity, the velocity of the pinacone forma- 
tion thus becomes proportional to the alcohol concentration; how 
many molecules of the ketone act simultaneously cannot be ascer- 
tained in this manner. As, however, pinacone and aldehyde are 
formed and as according to the above equation one molecule of 
alcohol is attacked simultaneously, the reaction scheme becomes : 

€,H,OH -— 2(C,H,),CO = C,H,0 + (C,H,),(CO), ?). 

In order to learn the temperature coefficient the ordinary tubes 
(16 mm. diameter) were enclosed and sealed into a second tube 
(244mm. internal diameter); the intervening space was filled with 
conductivity water and now two of these tubes were exposed to 
light as deseribed, one of them being kept at 25°— 28° and the 
other at 752—78°*). 

1) Here we have assumed that the change in concentration of the alcohol during 
each of the four experiments was so slight that it could be regarded as being 
constant; this, of course, is not correct and we really ought to have taken each 
time a portion from larger apparatus. In that case, however, the experiments 
would become much more complicated, because the light-quantilty did not then 
remain constant during the experiment. Hence, we have rested content with the 
above modus operandi which is sufficiently accurate for our purpose. 

*) For a mixture of ketone and benzhydrole we have proved this reaction scheme 
yet in another manner (see next communication). 

, 5) Compare Rk. LutHeR and F. Weiaerv, Z. phys. Ch. 58, 400 (190d). 


854 


TASB EGE aE 
ee eri |e reson 
j-— —--——- = = — — = 
Ist Series 
1 0.1 gr. benzophenone 0.09 gr. 
_; entirely converted 
2 | OP ses ; O23, 
3 | 050g "A 0.34, 
4 OWS, , 0.36, 
5 l— , 5 0:36) 
2nd Series 
1 1 gr. benzophenone 0.47 gr. 
2 Aa 9 0.49 ,, 
he F 0.49 ,, 
\3rd Series| 
1 0.1 gr.ochlorobenzophenone 0.09 gr. , 
5 | 025 , : sone entirely converted 
3 | 0.50 ,, 1 0.38, 
1 | OSs, %) 0.39 ,, 
Bie |) ng - 0.39 ,, 
6 2— ,, * 0.38 ,, 
ea iat ea oeoso.e 
Lan | ee 0.41 ,, 
ASB EVE. Ta: 
won | Gaveentiation/e] CRLOG in) | Gunster ore aes 
(CsH;)2CO per 25 ce. pig eS 
| 1 0.2527 gr. or 1 eq. 0.08 gr. 1 
2 05054 ar wean arc ayy 0.18 ., 2.25 
3 MOLOS ais ee 5 O36 4.50 
4 PAWN" 55 gy 13 sp 0.66 ,, 8.25 
5 © (pure alcohol) 0.69 ,, | 


855 


More accurate experiments were not considered necessary as we 
did not care for the absolute value, but only for the order of mag- 
nitude of the temperature coefficient. 

Adjacent to the jacketed tube was also suspended an ordinary 
tube to ascertain whether the presence of the jacket had any influence 
on the pinacone formation. 

The subjoined table II gives a survey of some series of experiments. 

From these results it follows that the method is sufficiently accurate 
for our purpose, the ketone reduction is indeed a_ photo-reaction 
with a small temperature coefficient; this still falls below the mean 
stated by PLornixkow') of 1,17 per 10°. 


TABLE Il. Time of exposure 2—3 days. 


a eee 
| K 
N° | Contents of inner tube 2 oes pinacone 4" 
| Ay 
a = = = ] =e ee = oe a —— =, 
Ist Series) | | \ 
1 gee (CgH5)2 CO in 25 ce. alcohol | 25°—28° | 0.45 gr. | 
without jacket | | | | | 
2 | SAS tends: with eee | 0.76 ,, | 
| {+ 50° | 1.06 
3 Ns Re Nile eae —78° 02a 
2nd Series) | | 
1 |. - . « . without jacket | 25°—28° | 0.44 gr. | 
2 1p 6-0 6 oo co WAU IECG: Fi ORK 
| | | 50° | 1.065 
3 WeMlerva tee ch SO my Skis, | ale =18e 0.96 ,, 
| | a 
\3rd Series 
1 Ips (CICgH4)3COin 25cc. alcohol | 25°—28? | 0.27 gr. | 
without jacket | 
Be cals ses 7 with jacket ne al 0.35, | 
|: a0 | 1.095 | 
Sea 7°—18" | 0.55 ,, | 
bs BL = 1 | 
|| | | 
4th Series 
| | 
1 . . . . . Without jacket | 25°—28° | | 0.24 gr. | 
2 | aeecee? Gel swithtjacket ij | 0.30 ,, 
| + 50° | | 1.10 | 
ue re eae Cas | | 0.50 ,, | 
: i, ao L 


1) Jon. Prornikow. Photochemische Versuchstechnik. p. 273 (1912), 


856 


That the temperature coefficient for orthochlorobenzophenone is 
really somewhat higher than for benzophenone seems to us rather 
probable, but this can only be ascertained by more delicate measu- 
rements '). 

The independence of the concentration and the very small tempe- 
rature coefficient now enables us to continue following this very 
simple method in the quantitative investigation as to the influence 
of the ketone to be reduced as well as of the reducing alcohol. 


Influence of the alcohol. 


The aleohols, as described above, were carefully dried over calcium 
and, after distillation, poured at once into the tubes containing two 
grams of ketone. These were then sealed and exposed to the light. 

These tubes were suspended at such a distance that they could 
not interfere with each other. 

The subjoined table gives two series of experiments, the first series 
was exposed for three and the second one for six days: particularly 
during the first days it was sunny spring weather. 

What strikes us here in the first place is the agreement in the 
action of the aleohols 2—6; the secondary propyl alcohol gets 
oxidised somewhat more rapidly. the amyl alcohol a little more 
slowly. In the latter case a strong yellow coloration sets in. 

Very much smaller is the velocity of the pinacone formation in 
the case of methyl and allyl aleohol; as no interfering yellow 
coloration occurred here and as the conditions were moreover quite 
equal, this different behaviour must be attributed to the particular 
position these alcohols occupy. 

Although we cannot yet enter here into an explanation of the 
process, if is obvious that the reduction of benzophenone will proceed 
all the more readily when in the conversion of alcohol into aldehyde 
(or ketone) more energy is set free. 

The absolute extent of this energy is unknown to us, but still 
some thermic data point to the existence of a parallelism in the 


1) The remarkably greater reduction velocity in the jacketed as compared with 
that in an ordinary tube, must be attributed to the larger quantity of light which, 
owing to refraction in the jacket filled with water, falls on the inner tube. In fact 
nothing could be noticed of this inner tube when the tube was entirely filled; it 
looked as if the alcoholic solution has the width of the outer tube. In harmony 
with this observation, it appears that the ratios of the velocities in the four series 
namely 76:45, 70:44, 35:27 and 30:24 do not greatly diverge and are about 
equal to the proportions of the sections of the outer and inner tube 24; 16. 
(Compare Lurner and Weicert |. c. p. 391). 


857 


TABLE Ill. 
lyst Nee 2 gr. benzophenone in 25 cc. panes Remarks 
1 | methyl alcohol 0.29 gr 
2 ethyl alcohol 0.84 ,, 
3 | n-propyl alcohol (Oates) — sy | faint yellow 
| coloration 
4 | sec. propyl alcohol | ORE | 
| | 
5 n. butyl alcohol On84 55 I 
6 _amylalcohol (Bp. 130 -133°), 0.75 _,, Sires yellows | 
7 allyl alcohol Ok25) | 
: Ratio | 
ies Sees | | | i’: 1 ete: 
= es ee 
iV methyl alcoho! | 0.49 gr. | 1.69 
| ea ethyl alcohol Vea ae | lhe wltgTA 
| | yellow coloration 
3f | n. propyl alcohol alts} a ea not much | 1.75 | 
| | increased 
4’ sec. propyl alcohol L605; 1.58 
; x ( yellow coloration) 
6 amyl alcohol (a. ab.) 1.05: |; par acre | 1.40 
I solr ea allyl alcohol Q:42e 6 1.68 


velocity of the reduction and the extent of the difference of the 
molecular heat of combustion of aleohol and the correlated aldehyde 
(or ketone). 

The greater this difference the more energy will be represented 
by the hydrogen atoms playing a role in that transformation. 

As the heats of evaporation of the alcohols on one side and of 
the aldehydes on the other side do not sensibly differ and as all we 
require lere are a few figures for comparison, a correction for this 
may be omitted here. We then find for these differences (according 
to data from the tables of Lanpoir-B6rnstein-Rota). (See table IV.) 

The heat of combustion of acraldehyde is not known, neither 
that of formaldehyde. There is, however, a statement as to meta- 
formaldehyde: if from this one calculates the molecular combustion 
as if it were a monomeride, the difference amounts to 47 cal. As, 
however, this also includes the heat of polymerisation the difference 
is presumably considerably less than 47 calories, 


858 


TABLE IV. 
a = ees vee 
3 = methyl alcohol—(meta)formaldehyde lwernss 47.0 cal. 
e = ethyl alcohol—aldehyde 47.075; 
5 g n. propyl alcohol—propionaldehyde 505 0ieny 
g 5 sec. propy: alcohol—acetone SOs 
2 r amyl alcohol (?)—valeraldehyde Ac O las 


The two series of experiments of table II] were started at the 
same moment, the first was investigated after three and the latter 
after six days; when the converted quantity of substance is proportional 
to the quantity of light and no secondary hindrances occur, the 
proportion of the quantities of pinacone at each of the numbers 
1:1’, 2:2’ ete. must be the same; these ratios have been inserted 
in the last column of the second series. 

We notice that this ratio is indeed almost constant except in the 
ease of amy! alcohol, where a hindrance in the form of an increasing 
yellow coloration is distinctly observed. 


Influence of the ketone. 


The tubes were filled with solutions of one gram of ketone in 
50 ce. of absolute ethyl alcohol. Two series were exposed simulta- 
neously to the action of the light; the first was investigated after 
three, the second after six days. Some pinacones remain very long 
in supersaturated solution, hence the alcohol was always distilled 
off and the residue shaken with 80°/, aleohol so as to remove all 
unconverted ketone 

The subjoined table V gives the results obtained and the ratios of 
the velocities with those of the benzopinacone formation as unit. 

Table VI gives a similar double series; most of the ketones 
investigated here were not attacked. 

Table VIL gives a survey of the results obtained in amyl alcohol 
as solvent and as reducing agent. 

1st. The velocity of the pinacone formation, according to this 
survey, is greatly dependent on the nature and on the position of the 
substituent. As regards the nature, there is only one group (the 
methyl group on the two para-positions (N°. 7)) that appears to 
accelerate the reduction velocity somewhat, for the rest the substitution 
causes a decrease in velocity. 

This decrease is strongest when the substituting group isa phenyl 


859 


TA'BLE V. 
| Quantities of pimacone Ratio. | Ratio of the Re- 
No.| Name of the ketone SeriesI Series i Series I Series I | with tat obo 
In grams In millimols. (CoB CO as unit 
1 | benzophenone 0.41 0.85 1.12 2.32 2.05 io 
2 | 2 chlorobenzophenone 0.12 0.25 0.28 0.58 2.07 0.25 
3 | 3 chlorobenzophenone 2 +0.10 - 0.23 — +0.1 (from II) 
'4 | 4 chlorobenzophenone 0.32 0.75 0.74 1.73 2.34 0.66 
5 | 4 methoxybenzophenone 0.39 0.80 0.92 1.88 2.04 0.82 
6 | 4 methylbenzophenone 0.41 0.86 1.04 2.18 2.09 0.93 
7 | 44’ dimethylbenzophenone 0.48 0.95 (off)| 1.19 — a 1.06 
8 | 4 bromobenzophenone 0.51 0.98 (off) 1.— _ — 0.90 
9!) | 44’ dichlorobenzophenone 1% 0.73 — 1.45 =| 0.63 (from II) 
10 | 2.2.4.4’ tetrachlorobenzoph. 0.22 0.47 0.34 | 0.72 7512 | 0.30 
11 | 2 chloro 4’ methyl ne | 0.27 | 0.55 0.58 | 1.18 2.03 0.52 
12!) | 4 chloro 4’ methyl " 0.19 | 0.70 0.41(2), 1.50 3.66(?), 0.64 (from II) 
| 
ABE Vie 
13. benzophenone 0.85 0. og (oft 2ESO | _ — 1 
14!) | 4 phenylbenzophenone To | _ | _ — 0 
15 | phenyl-~-naphtylketone a2 | es = | bs ue 0 
16 | phenyl-3- 5 _ _ De el es — 0 
17 | 2 methylbenzophenone _ == re es ere _— 0 
18 | 3 methylbenzophenone | 0.80 | 0,96 (off) 2.03 — = 0.89 
19 | 2.4.2’.4’ tetramethyl ,, ae a = | — = 0 
20 | fluorenone } — |e Tels — 0 
te | 
TABLE VII. Amy! alcohol as solvent. 
21 | benzophenone ) Osis 0.97 (off) 2.05 | -- 22 1 
22 | 2 chlorobenzophenone | 0.22 | 0.33 | 0.51 0.76 1.49 | 0.25 
23 | 4 chlorobenzophenone 0.65 0.96 1.49 | 2.20 1.48 | 0.72 
24 | 4 methylbenzophenone 0.74 0.96 (off), Hash} |) — | 0.91 
25 | phenyl «-naphthylketone | _ | _ | _ | — — | 0) 


') These ketones had not entirely passed in solution in the alcohol. 


S60 


vroup, because 4-phenylbenzophenone (14) and the two phenyl- 
naphthylketones (J5 and 16) are not reduced. 

Halogen atoms and methyl groups do diminish the single substitution, 
but (with one exception) do not prevent the same. Para substitution 
has the least influence, ortho the greatest; this, however does not 
apply to the chlorobenzophenones (3), so that we can hardly speak 
of a universal rule. 

The symmetry of the molecule seems to accelerate the velocity. 

Whereas the 4-methylbenzophenone has a smaller velocity than 
the benzophenone (5), the 4.4’-dimethylbenzophenone has a somewhat 
greater one. The fairly considerable decrease in velocity in the 
4-chlorobenzophenone (4) is not continued in the 44’-dichlorobenzo- 
phenone (9). In connexion with the considerable decrease in the 
2-chlorobenzophenone (2) that in the 2.2’.4.4’-tetrachlorobenzophenone 
(10) is unexpectedly high. 

A remarkable fact is the slight influence of the methyl group on 
the meta position (18) in regard to the great one of the chlorine atom (8). 

2nd. Of more importance is the fact that the aleohol, the reducing 
agent, is of very secondary significance as regards the ratio of the 
reduction velocities; this is shown from the comparison of tables 
V and VII. The ratio of the velocities in ethyl and amyi alcohol 
is practically the same. We have completed these observations with 
a few on methyl and propyl! alcohol, selecting methy! aleohol because 
the velocities therein are generally much less, whereas o-chloro- 
benzophenone with benzophenone were compared as ketones, because 
the velocities in ethyl (and amyl) alcohol differ strongly. 

The subjoined table VIII gives a survey of the results. 


thyl ketone | § 


TABLE VIII. 
fi kee = eras We ee: 
Sol. C,H5;OH, |) Sol.C;H,,OH, | Sol. CHg OH, || Sol. nC3H;OH, 
Ist Series |; 3rd Series || 4th Series 5th Series 
| ~-— |. |X 
Quantity Quantity | | Quantity | Quantity 
| in Ratio in Ratio | in | Ratio in Ratio 
| m.mols. | m.mols, m.mols. | | m.mols. 
| Benzophenone|} 2.32 | 1.0 2.05) 91 ek Art |) “2.93. ad 
/2Chloro_,, 0.58 0.25) 0.51 (0.25 | 0.46 | 0.24 || 1.08 | 0.27 
| | | 
(Ne . | 1.73 | 0.66 || 1.49 | | 0.72 | 
[4methyl | 2.18 | 0.93 1.88 | 0.91 
| | ] | 
| phenyl «-naph- } 9 | eel 0 
| | 
| 


861 


First of ali it follows from this constant ratio that the hefore is 
prominent in the photo-reaction, that this passes into a photo-active 
condition. Further, that the diverse ketones are activated in a 
perfectly analogous manner in such a way that either a number of 
molecules (the same for all ketones) become photo-active, which molecules 
then react with the alcohol with a velocity specific for the ketone; 

or, a number of molecules specific for each ketone becomes 
activated which, with a definite velocity which is independent of 
the ketone, dehydrogenises the alcohol. 

A choice from these alternatives can only be made by a further 
study of the photo-reaction. 

The active light of the ketone reduction. 

The first attempt to ascertain the position of the active light in 
the spectrum has been made by Cramician and Sinper'). They in- 
vestigated, for instance, the reduction of benzophenone and alcohol, 
employing two photo-filters. 

As a red photo-filter was used a cold saturated solution of fluo- 
rescein in alcohol (thickness of layer 15 mm.) which extinguishes 
all light to 0.510 @; by adding gentian-violet the absorption could 
be raised to 0.620 «. 

As a blue filter served a 10°/, solution of cobalt chloride in alcohol 
which transmits rays of a wavelength less than 0,480 uw; a ereen 
band at + 0,560 w and a red one at + 770u remain, however, 
unextinguished. They arrive at the result that all the reactions with 
which they were engaged, took place under the influence of blue 
light. We have used a larger number of photo-filters and carried 
out the research in jacketed tubes; the inner tubes were those which 
were used by us in the other experiments; the intervening space 
was 15 mm. Above the liquid in the jacket the outer tubes were 
covered with black lacquer, so that none but filtered light could 
penetrate into the inner tube. 

As photo-filters were selected : 

I. Red: aqueous solution of chrysoidin *). 

Pe Greeny:) ©; » 9, potassium dichromate + acid green 
B. extra. ?) 
Blue and violet. 
ILI. 10°/, aleoholic solution of CoCl,. 
IV. Cold saturated aqueous solution of erystal violet 5 B. O.?). 
VALS 2 » 5 » acid violet 4 B. N. ?). 
VI. Solution of iodine in CCl,. 


1) B. 35, 3593 (1902) 
2) Colouring matters from the “Gesellschaft f. chem. Ind. Basel’. 


862 

In agreement with that found by Cramiciay and Sitper for the red 
fluorescein filter we found that the filters I and Il which only 
red (690—598 we) or red and green (> 500 uy) absorbed 
all actinic rays. 

Also V, which besides red rays of about 700 ue still transmitted 
blue and violet > 483 nu, completely prevented the reduction in the 
inner tube. On the other hand an important reduction took place with 
the filters 11], 1V, and VI which transmitted rays to the extreme, visible 
violet + 400 ay. 

The series of experiments were conducted in this way that a set 


transmit 


of four jacketed tubes with photo-filters were exposed to sun-light 
for some days in front of the white screen: the results are contained 
in the subjoined table. 


TABLE Ix. 
: ee | Quantity | = 
7 5 : ; i | Photo- of 
N>. | Ketone in the inner tube | filter | pinacone Remarks 
Poel ae ee cee eae oe 
list Series 
| 1 2 gr.benzophenone in 25 cc,C,H;OH I 0 
| 2 | : Il 0 
entirely 
3 ie il 2 converted 
4 We IV 0.67 
| . 
2nd Series) 
5 | « 4 Ill 0.85 | From the com- 
| parison of the 
6 Jab, 0 | figures for III 
| | and IV with the 
7 ne i AL 0.48 controlling tube 
with conduct- 
(conduct- ivity water it 
Sma . (2. ivity 1.28 | appears that 
| ? water there always 
| | takes place a 
ail as : Shae partial absorpt- 
I3rd Series ion of the actinic 
rays; this, how- | 
9 2 gr. o-chlorobenzophenone lll 0.33 ever, isrelatively — 
| small and is pro- 
10 Vv 0 | bably based on 
a general ab- 
11 VI 0.28 sorption, which 
| in a_spectros- 
(conduct. | copic investigat- 
\, 2 | . |. ivity 0.42 | ion was readily 
ri observed. 


eel 


863 


Now with this method we can only get a very rough determination 
of the position of the active region, still it appears that the active 
rays are presumably situated in the violet and have a wavelength 
smaller than + 480 uu. In order to see whether in the beginning 
of the ultraviolet active rays were still present, a small jacketed 
tube was constructed from quartz, the alcoholic benzophenone solution 
was put into the inner tube and in the jacket a cold saturated 
solution of nitrosodimethylaniline') which absorbs all visible violet 
and blue rays and transmits ultra-violet ones of 400—280 uu. 

Neither in sun-light, nor in front of the quartz lamp did any 
reduction set in; from this we could conclude that the active rays 
were not situated in the ultra violet, but in the visible spectrum 
< 480 and > 400 au. 

A fortunate incident now came to our aid when we were engaged 
in determining the correct position of the active light. 

We had noticed that the ketones were converted with compara- 
tively great rapidity into pinacones by means of the HerAvs quartz- 
mercury lamp. ‘ 

The mercury spectrum must thus contain a great quantity of the 
chemically active rays. This spectrum exhibits a very intensive blue 
line at 436—434 wu and two violet ones at 407,8 uu and 404.7 wu?), 

Photo-filter V completely removes the violet lines and leaves the 
blue ones unchanged; as this filter in sunlight as well as in front 
of the quartz lamp prevents all conversion of benzophenone as well 
as of o-chlorobenzophenone, and as we have noticed that the ultra- 
violet light of the lamp is inactive we may conclude that the active 
light for the photochemical reduction of the aromatic ketones is 
situated in the extreme end of the visible violet. 

The fact that the nature of the source of light has no principal 
influence on the reduction process is shown from the subjoined table, 
in which are given the ratios of the quantities of pinacone that are 
formed from diverse ketones when exposed either to sun-light or 
mercury-light. 

The exposure to mercury-light was carried out by placing a solution 
of 0.5 gram of ketone in 15 ce of ethyl alcohol at a distance of 
5 em from and parallel to the quartz lamp and exposing these for 
10 hours; hence, the quantity of light was approximately the same 
for all ketones. 

The close agreement of these ratios also renders it probable that 


1) Compare PLornixow etc. p. 19. 
2) Lenmann, Plays. Zeitschr. 11, 1039 (1910), 


Proceedings Roya! Acad. Amsterdam. Vol. XVII. 


864 


TMA E IE, 0G 
3 | ene of pinacone a Semen  Gaenaes of 
to Hg light pinacone on 
No. Name of the ketone | in m.mols. Gite ligtt with beng 
in grams benzopinacone pinacone as 
as unit unit 
1 benzophenone 0.35 1 1 
2 2 chlorobenzophenone 0.10 0.23 0.25 
3 4 chlorobenzophenone 0.30 0.70 0.66 
4 2 methylbenzophenone 0 0 0 
5 4 methylbenzophenone 0.34 0.89 0.93 
6 phenyl z-naphthylketone 0 0 0 
7 fluorenone 0 0 0 


the active rays are situated for the greater part at 407.8 and 404.7 wa *). 
The action of light on mixtures of ketones. 


The phenomena observed by us during the exposure to light of 
ketone mixtures in absolute alcohol divulged a very strong mutual 
influence. 

In order to better understand these observations, the following 
should precede: 

We have noticed that the chemically active light comprises a very 
limited part of the spectrum, yet, therein are rays of different 
frequency and intensity. 

A. We can now suppose that each of the ketones present wants 
its own active rays without absorbing rays intended for the other 


ketone; then — as the pinacone formation is independent of the 
concentration — there will have formed in the tube with the mixture 


the sum of the quantities of pinacone that are formed in the separate 
tubes under the same conditions. 

Those quantities within certain limits must also be independent 
of the proportion of the concentrations of the ketones in the tube 
containing the mixture. 

1) Presumably, the action is in a high degree selective, as a layer of 3 dm 4°/, 
benzophenone in absolute alcohol certainly caused a very distinct fading of these two 
mercury lines, whereas nothing could be noticed of a curtailing or fading at the 
violet side of the are lamp spectrum through that same liquid layer. We attach, 
moreover, not much value to this subjective observation, for only an accurate 
spectrophotometric investigation of the absorption spectra of the ketones can 
properly delermine the connexion between absorption and chemical action. 


865 


b. As soon, however, as rays for the one ketone are also con- 
sumed by the other one, the quantity of pinacone will be less than 
the sum in question and, moreover, the proportions of concentrations 
will no longer be a matter of indifference. 

For in the layer where the photo-reaction takes place each molecule 
of the one ketone requires a part of the light-energy also wanted by 
the second ketone, so that the hindrance experienced by the latter 
will become greater when its relative concentration gets less. 

C. The extreme case would be that both ketones require just 
the same rays; we should then obtain a quantity of each of the 
ketones which in equimolecular concentration is equal to half the 
quantity that forms in the tube with the separate ketone (always 
supposing that no other obstacles occur). 

The phenomena recorded by us are now best understood from 
the supposition B; a ketone does require specific rays from its 
neighbour. Some of the observations approach to A, others to C, 
some even exceed this extreme case, showing that the action is 
more complicated than was at first supposed, as will appear from 
the subjoined tabulated survey. 


HAGE I ENeX 
| Ist | Solution of 2 gr. of o-chlorobenzo- ind50cc, Quantity 
/Series phenone and varying quantities of Aohal pinacone Remarks 
No. phenyl z-naphthylketone in gr. 
} | og nr 
| 1 |2 gr. o-Clbenzophenone pure 0.84 |S, ES 
| ; ; ae 
ae 62 * +-0.1 gr. phenyl z-naphthylketone 0.30 5 5305S 
| eoFag 5 
3 - SOIR 5 , PO) ea eee aI) 
coy ee! vas 
4 +0,50 , i 0 Sesgeco. 
” s} » tr oor aS 
- 
5 ” ail ” » ” 0 ve Sd%a 
ea c& oc 
° ees iS = 
= fe 3 s A 
v = 
esezas 
zie As above o-Cl benzophenone and varying Quantit 
jopaccite s above o- one ¢ ary uantity) , spe 
pees quantities of o-methylbenzophenone pinacone Remarks 
| i = BAN RIN : 
| 1 | 2gr. o-Cl benzophenone pure Ose 
2 a +-0.1 gr.o-CHg3benzophenone 0.36 
|| ees és + 0.25 Fe 0.30 As above 
| 4 | . + 0.50 ; 0.26 
j | 
fect i + 1 ; | 0.15 


866 


We notice that when one of the ketones does not get reduced it 
exerts a very powerful retarding action on the reduction of the 
other. ketone. 

This action, particularly with phenyl-e-naphtylketone is much 
more important than we should expect even in the extreme case C; 
besides the elimination of the chemically active rays, the molecules 
of the naphtylketone must cause an impediment, which may, perhaps 
be put on a par with the obstruction caused by oxygen in the 
photo-halogenations. 


TABLE XII. 
ree ewes - 
p> 3 Seo ol ee 
Solutions of various ketones, which are | 5 oo Re SEs 
N : : [See o2w | oes] Remark 
reduced separately in 50 cc. solution. SSS Bae | sso 
ole m°S|ros 
| ° = 
; moe eT be eee lll 3 
ee ee 
WN) | | = cH 
1 2gr. benzophenone Neel ite |p - Boe. 
| | =%27y2 
2~|2 > + 2gr.0-Cl benzophenone | 2.31 | 4.16 5 Eta 
2.37 3.8) efea 
Su ane > +1» > 2ST} | 3.46 8 M4 ot oe 
oLor 
7 : = es = 2 
2f | sige 
jan oo 
1 | 2gr. benzophenone 166" || 1667) a E Bus g 
| : Qa, 
2 |2> > +2gr.pClbenzophenone 2.18 9.19 | | S°5E 
2.76 1.2: Saas 
3 |2 > +1» > 1.69 \ 3.19 | fees 
os a 
2 ; ee (S788 
ze | 338e 
oO oO | ats 
a | eels 
1 2gr. benzophenone . 0.85 0.85 —_ = 5 2 ae 
WS Sw 
Qu | 2s > + 2gr.pBrbenzophenone | 1.65 | 23.9 | |= ae iS 
1.95 19.0 | w@E& 
3 12> r iis ‘ 1.05 |) 11.4 || \oe 8 


From Table XII it appears that, in the case when both ketones 
are reduced, we have demonstrated a considerably less impediment 
than in the case that one of them is not reduced. Still, there is 
always a negative influence, we obtain in all cases a quantity less 
than the sum of the quantities which we should have obtained, in 
separate tubes; we are always dealing with case B. 

In this we notice the smallest mutual hindrance in the mixture 
of benzophenone and o-chlorobenzophenone, yet we notice plainly 
that the impediment increases when one of the ketones is present 


in large excess (18tseries N’. 3) and that in such a case that present 
in the smallest amount is the most strongly impeded. Much more 
pronounced is the hindrance observed with mixtures of benzophenone 
and p. Cl- or p. Br-benzophenone; the sum of the pinacones remains 
here far below the calculated quantity. The halogen ketone has as 
a rule a stronger impeding action than benzophenone, for even in 
smaller quantities than the molecular ones (N°. 2 of the three series) 
the halogen pinacone in the mixture is predominant. Only with a 
considerable excess of benzophenone the halogen pinacone is repelled 
and mostly so in the cases where the greatest hindrance is present 
(compare N°. 3 of the three series). 

We thus find in rough traits what we could expect; there occur, 
however, particularly when one of the ketones is not reduced 
separately, such great hindrances that they cannot be satisfactorily 
TABLE XIill. 


| Quantity 


Contents inner tube | Contents outer tube : Quantity of 
eer | Pinacone |pinacone in the 
| N.|2 gr. benzophenone in| 50 cc. abs. alcoholic | Ps inner tube with | 

< ; ; | #38 Y the blank tube 
| 20 ce. abs. aluohol | solution of 4 grams: 2 ej aan tit 

| : 

wn —- = = = = == = = 
~ Vv 
,n°s 
25 

n } 

Te | alcohol (blank-exper.) | 0.64 — | 1.— 
2 p CH; benzophenone 0.28 | 0.66 0.44 
aes | oCl benzophenone | 0.18 0.19 0.28 
| 
| 4 | phenylz naphthylketone trace 0 | trace 

=F —— 77 == 4 
ro | 
Sis] 

N VU) 

a 
Hele| alcohol (blank-exper.) 1.05 - 1.— 
| | 
Hee o CH3 benzophenone | 0.50 0 0.48 

3 ‘phenyl-naphthylketone) 0.28 0 0.27 

4 fluorenone 0 0 0 
| 

wi a ———_=. ci aoa = 73 
aeig) 

6 5) 

w) | | 

1 | alcohol (blank-exper.) | 0.79 | — 1.— 

2 p Brbenzophenone | 0.42) 1,18~ 0.54 

3 p Cl benzophenone 0.38 | 0.83 0.47 


| 4 benzophenone 0.29 | 0.93 0.37 


868 


explained in the above cited manner. There seems to be a connexion: 
here between the extent of the impediment and the non-appearance 
of the photo-reduction. 

Now, in order to eliminate the hindrance which might eventually 
take place owing to the mixing, the oft-quoted jacketed tubes were 
filled in such a manner that in the inner tube was alivays inserted 
a definite ketone and in the jacket diverse other ketones, 

The light then first traversed a + 2 mm. thick layer ofa ketone 
then to exert ifs action on the benzophenone; in this way we could 
form a better opinion as to the absorption of rays of light by the 
one ketone (in the jacket) which were needed for the other ketone 
(in the inner tube). 

There exists no doubt that a// ketones absorb actinic rays intended 
for the benzophenone; the degree of this absorption is certainly 
very different and specific. 

The ketones which were attacked in the jacket were, during the 
experiment, reduced in concentration, so that the conditions for the 
reducing of the benzophenone in the inner tube gradually became 
more favourable; this causes, however, that we can only consider 
as fairly comparable the experiments where no reduction takes place 
in the jacket. Hence, a few ketones have been placed in the jacket 
in benzene solution whilst in the inner tube was again present a 
solution of 2 grams of benzophenone in 20 ec. of absolute alcohol ; 
the following result was thus obtained: 


TVAVB EE exw. 
In the inner tube | In the jacket a Quantity of 
N°.! 2 gr. (CgsHs),CO | N/4 benzene solu- | pinacone in the | Remarks 
in 20cc. abs. ale. tion of itmer tube. 
1 — (blank) Pa 134e 91%) 1/50 | 
| | | The benzene 
2 | benzophenone | 0.45 | OFS4 ea | solutiontaniaer 
a i a | i jacket was al- 
3 o-chloro | 0.53 0.40 | | Ways coloured 
| S42 ~ pale yellow 
| as | Pp 0.34 0.25 | which colour 
rae | : é again faded in 
| 5 p-methyl » 0.40 0.30 the dane 


It appears that several ketenes absorb rays of light which effeet 
the benzophenone activation, even when they are dissclved in 
benzene. 

The reversible yellow coloration of this benzene solution, however, 
tells us to be careful, for the activated ketone can form with benzene 


R69 


a light-sereen, thus causing the absorption effect to be greater than 
when the ketone had been present in alcoholic solution. 

In each case a circumstance oecurs owing to which the phenomenon 
becomes more complicated, so that from these last experiments we 
may at most draw the conclusiun that rays of light are indeed always 
absorbed by the one ketone, which the other required for the oxidation 
of alcohols. 


The most powerful absorbing ketones appear mostly — but not 
always — to oxidise the alcohol slowly or not at all, so that we 


gain the impression that a liberal absorption does take place, but 
that the possibility of the setting in of a reaction and its velocity 
does not only depend on the aleohol, but in a great measure on 
the ketone. 

It speaks for itself that the experiments on this almost quite 
unexplored region can only bear a very provisional character ; still 
we believe we have attained, with very siinple means and methods, 
some results which will prove of importance for the insight into 
the photochemical reactions. 

For the moment, however, we wish to refrain from an attempt to 
explain the phenomena observed until more accurate spectrophoto- 
metric data are at our disposal. 


SUMMARY. 


I From aromatic ketones and alcohol are formed, in the light, 
exclusively pinacones; these latter are, therefore, the products 
to be first isolated in the reduction. Hydrols are, in the reduct- 
ion of the aromatic ketones, always formed secondarily (see 
Proc. XVI 91 and 962) either from the pinacones or from 
the primarily formed half pinacone molecules. 

II 1. The photo-reduction - of the ketone by alcohols was studied 
by exposing simultaneously to the light a set of tubes of 
equal dimensions and filled with equal quantities of liquid, 
thus causing the light-quantity (i.t) for each object of a 
serial experiment to be equal. 

2. The velocity of the pinacone formation appeared to be inde- 
pendent of the concentration of the benzophenone and propor- 
tional to the concentration of the alcohol. Hence, it satisfied 
the equation : 


d pinacone 


—= KT. [alcohol 


and, therefore, the reaction scheme: 


dt 
2 ketone + alcohol = pinacone + aldehyde, 


870 


3. The temperature coefficient was small: 1.06—1.11 for 10°. 

4. The velocity of the pinacone formation is greatly dependent on 
the aleohol; for instance, the methyl aleohol and the allyl 
aleohol were oxidised much more slowly than other primary 
and secondary alcohols. 

5. The velocity of the pinacone formation is greatly dependent 
on the ketone, the benzophenone is attacked rapidly, most of 
the ketones as yet examined less rapidly, many not at all. 

6. The ratio of these velocities in different alcohols is constant. 

7. The aetive light of the ketone reduction is sure to be situated 
in the spectrum between 400 and 480 «qe and very probably 
in, or adjacent to, the rays 404.7 and 407.8 of the mercury 
quartz lamp. 

8. The ratio of the velocities of the pinacone formation in sun- 
light and in mercury light is the same. 


<2 


When two ketones are present simultaneously one of them 
absorbs a part of the rays required by the other ketone; this 
also appears when the light passes through a solution of the 
one ketone and falls on that of the other. 

Particularly in the case of the powerfully absorbing ketones 
the hindrances are stronger than was to be expected. 
Delft, October 1914. 


Physics. — “Simplified deduction of the formula from the theory 
of combinations which PLanck uses as the basis of his radiation- 
theory.” By Prof. P. Eurenrest and Prof. H. Kammrtincu ONNEs. 


(Communicated in the meeting of Oct. 31, 1914). 


We refer to the expression 
, (N—1+4P)! 
oN ™ ae )! (4) 
ted PN—1)! 


which gives the number of ways in which .V monochromatic reso- 


nators f,, R,,... Ry may be distributed over the various degrees 
of energy, determined by the series of multiples 0, ¢, 2¢... of the 


unit energy ¢, when the resonators together must each time contain 
the given multiple Pe. Two methods of distribution will be called 
identical, and only then, when the first resonator in the one distri- 
bution is at the same grade of energy as the same resonator in the 
second and similarly the second, third,.... and the Vth resonator 
are each at the same energy-grades in the two distributions. 
Taking a special example, we shall introduce a symbol for the 
distribution. Let NV = 4, and ?=7. One of the possible distributions 


871 


is the following: resonator A, has reached the energy-grade 4e (R, 
contains the energy 4s), R, the grade 2s, R, the grade Oe (contains 
no energy), R, the grade «. Our symbol will, read from left to right, 
indicate the energy of R,, R,, R,. R, in the distribution chosen, and 
particularly express, that the total energy is 7s. For this case the 
symbol will be: 


(EES 0FHO00H] 


or also more simply : 


ceeeOreQOr]] 


With general values of .V and P the symbol will contain P? times 
the sign ¢ and (.V—1) times the sign O'). The question now is, 
how many diferent symbols for the distribution may be formed in 
the manner indicated above from the given number of ¢ and O? 


The answer is 


(N—1+4P)/ 


el ee ea) 


Proof: first considering the (M—1-+ P) elements ¢...2, 0...0 
as so many distinguishable entities, they may be arranged in 


(NGA OP Re tytn ee na 2, 
different manners between the ends ][ [[. Next note, that each time 
(NMRA PROT em inl ee UR (3) 


of the combinations thus obtained give the same symbol for the 
distribution (and give the same energy-grade to each resonator), viz. 
all those combinations which are formed from each other by the 
permutation of the P elements ¢7*) or the (N—1) elements 0. The 
number of the different symbols for the distribution and that of the 


1) We were led to the introduction of the (N—1) partitions between the NV 
resonators, in trying to find an explanation of the form (NV — 1)! in the denomi- 
nator of (A) (compare note 1 on page 872). Pranck proves, that the number of 
distributions must be equal to the number of al! ‘‘combinations with repetitions 
of N elements of class P” and fur the proof, that this number is given by the 
expression (A), he refers to the train of reasoning followed in treatises on com- 
binations for this particular case. In these treatises the expression (A) is arrived 
at by the aid of the device of “transition from nton-+-1”, and this method taken 
as a whole does not give an insight into the origin of the final expression. 

*) See appendix, 


872 


distributions themselves required is thus obtained by dividing (2) by 
(3) q. e.d.*). 


AGP AE BENG DFIEXe 


The contrast between Purncx’s hypothesis of the energy-qrades and 
Einstein's hypothesis of energy-quanta. 


The permutation of the elements ¢ is a purely formal device, just as the per- 
mutation of the elements 0 is. More than once the analogous, equally formal device 
used by PLANCK, viz. distribution of P energy-elements over N resonators, has by 
a misunderstanding been given a physical interpretation, which is absolutely in 
conflict with PLANCK’s radiation-formula and would lead to Wien’s radiation formula. 

As a matter of fact PLANCK’s energy-elements were in that case almost entirely 
identified with Ernstern’s light-quanta and accordingly it was said, that the difference . 
between PLANcK and Erysrein consists herein that the latter assumes the existence 
of mutually independent energy-quanta also in empty space, the former only in 
the interior of matter, in the resonators. The confusion which underlies this view 
has been more than once pointed out *). EINSTEIN really considers P similar quanta, 
existing independently of each other. He discusses for instance the case, that they 
distribute themselves irreversibly from a space of NV, cm’ over a larger space of 
Ng em® and -he finds using BoutzMan’s entropy-formula: S = klog W, that this 
produces a gain of entropy %): 


2 N,\P 
S— s, = ley (2) pete So. (3) 


ai 

1) It may be added, that the problem of the distribution of N resonators over 
the energy-grades corresponds to the following: On a rod, whose length is a mul- 
tiple Pe of a given length -, notches have been cut at distances ¢, 2e, ete. from 
one of the ends. At each of the notches, and only there, the rod may be broken, 
the separate pieces may subsequently be joined together in arbitrary numbers and 
in arbitrary order, the rods thus obtained not being distinguishable from each other 
otherwise than by a possible difference in length. The question is, in how many 
different manners (comp. Appendix) the rod may be divided and the pieces distri- 
buted over a given number of boxes, to be distinguished from each other as the 
Ist 2nd,.... Nth, when no box may contain more than one rod. If the boxes, 
which may be thought of as rectangular, are placed side by side in one line, they 
form together as it were an oblong drawer with (N—1) partitions, formed of two 
walls each, (comp. the above symbol in its first form, from which the second 
form was derived by abstracting from the fact, that each multiple of < forms one 
whole each time), and these double partitions may be imagined to be mutually 
exchanged, the boxes themselves remaining where they are. The possibility of this 
exchange is indicated by the form of the symbol chosen. 

As a further example corresponding to the symbol we may take a thread on 
which between P beads of the same kind, (N—1) beads of a different kind are 
strung, which divide the beads of the first kind in a Ist, 2nd... Nth group. 

*) P. Enrenrest, Ann. d. Phys. 36, 91, 1911, G. KrurKow, Physik. Zschr. 15, 
133, 363, 1914. 

3) A. Eysrern, Ann. d. Phys. 17, 132, 1905, 


Sie 

i.e. the same increase as in the analogous irreversible distribution of P similar, 
independent gas-molecules, for the number of ways in which P quanta may be 
distributed first over N,, then over Ny cells in space, are to each other in the ratio 
INERT tas 5. Cate oe ee (O) 
If with PLanek the object were to distribute P mutually independent elements 
« over N resonators, in passing from N, to Nz resonators the number of possible 
distributions would in this case also increase in the ratio (=) and correspondingly 
the entropy according to equition (z). We know, however, that PLANncK obtains 

the totally different formula 
(V,—1+4+ P)! Ned SI 
(N= 1)! P! (N= 1) P! (”) 
(which only coincides approximately with (@) for very large values of P) and a 
corresponding law of dependence of the entropy on N. This can be simply 
explained as follows: PLancKk does not deal with really mutuaily free quanta < , 
the resolution of the multiples of ¢ into separate elements <, which is essential in 
his method, and the introduction of these separate elements have to be taken 
“cum grano salis”; it is simply a formal device entirely analogous to our permut- 
ation of the elements = or O. The real object which is counted remains the number 
of all the different distributions of NV resonators over the energy-grades 0, ¢, 2, ... 
with a given total energy P:. If for instance P= 3, and N=2, Erysretn has to 
distinguish 23— 8 ways in which the three (similar) light-quanta A, B, C can be 

distributed over the space-cells 1, 2. 


ae B= €C 
Teleie mete 1 
Hee tari eee 
i te eee 
Wet, 22 
op Bagh See 
VIP 2p yet. 2 
Vil 2a ae 
VII | 2-2 2 


PiaNncK on the other hand must count the three eases II, Ill and V asasingle 
one, for all three express that resonator R, is at the grade 2, R, at<; similarly 
he has to reckon the cases IV, VI and VII as one; R, has here ¢ and R, Qe. 
Adding the two remaining cases I (A, contains 3¢, Ry Oe) and II (R, has Oz, Ry Be) 
one actually obtains 

(N--1--P)! (2—1+8)/ 
Wren C= 37 
different distributions of the resonators R), R, over the energy-grades. 

We may summarize the above as follows ; Etysrrtn’s hypothesis leads necessarily 
to formula (z) for the entropy and thus necessarily to Wren’s radiation-formula, 
not PLANCK’s PLANCK’s formal device (distribution of P energy-elements < over 
N resonators) cannot be interpreted in the sense of Etysrern’s ligit-quanta. 


(December 24, 1914). 


Q Akademie van Wetenschappen, 


57 Amsterdam. Afdeeling voor 
Ads de Wis- en Natuurkundige 

Werk Wetenschappen 

pu. dL Proceedings of the Section 
Physical & Of Sciences 


Applied Sci. 


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